Astronomers found a giant wall of galaxies hiding in plain sight – MIT Technology Review

Astronomers have found one of the largest structures in the known universea wall of galaxies thats at least 1.4 billion light-years long. And given how close it is to us, its remarkable that we havent seen it before now.

What happened: An international team of scientists reported the discovery of the South Pole Wall in a paper published Thursday in the Astrophysical Journal. The structure is basically a curtain that stretches across the southern border of the universe (from the perspective of Earth) and consists of thousands of galaxies, along with huge amounts of gas and dust.

What do you mean by wall? Galaxies arent just strewn randomly throughout the universe. Along huge strands of hydrogen, galaxies collect into larger groupings of massive filaments, separated by giant voids of nearly empty space. Each filament is basically a wall of galaxies, stretching for hundreds of millions of light-years. Theyre the biggest structures in the known universe. Other identified structures include the Great Wall, the Sloan Great Wall, the Hercules-Corona Borealis Great Wall, and the Bootes Void.

Put together, these walls make up what astronomers call the cosmic web. Piecing together the cosmic web is one of the major pursuits of cosmologyit would not only tell us about the structure of the universe and its interior but could also help us better understand how the universe was formed and how its evolved over time.

Why is this one special? Its so close! The South Pole Wall is just half a billion light-years away. In fact, this is part of the reason it was so hard to find until nowit is situated right behind the Milky Way galaxy, in a place called the Zone of Galactic Obscuration, where the galaxys brightness effectively kept the wall shrouded in plain sight.

So how was it found? Cosmological surveys are often done by measuring objects redshift: the speed at which those objects seem to be moving away from Earth thanks to the expansion of the universe. The faster an object is receding, the farther away it is.

The team behind the South Pole Wall discovery did redshift observations as part of their survey of the sky, but they also added measurements of the velocity of certain galaxies, which illustrates how they gravitationally interact with one another. This technique can alert astronomers to unseen masseswhile its normally used to investigate dark matter, it can also just highlight masses obscured by bright light. Using this data, the researchers were able to map out the South Pole Wall for the first time.

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Astronomers found a giant wall of galaxies hiding in plain sight - MIT Technology Review

Your best chance to see Jupiter this year – Astronomy Now Online

Mighty Jupiter, the king of the planets, comes to opposition at 08:00 UT on 14 July, the moment when it lies opposite the Sun in sky at a distance of 619.4 million kilometres (384 million miles), or 4.139 astronomical units. This is the most favourable time to observe the so-called superior planets (those apart from Mercury and Venus, which are termed inferior planets).

Jupiter, by far the Solar Systems dominant planet and the one that offers the most to observers of all levels or experience, is at its 2020 best on the nights of 13/14 and 14/15 July, when its a brilliant magnitude 2.8 beacon rather low in the southern sky among the stars of Sagittarius as soon as what passes for darkness as this time of the year descends. The presence of Saturn, the gorgeous ringed planet which comes to opposition itself on 20 July, lying just six to seven degrees to the east of Jupiter, adds greatly to the spectacle.

As Jupiter doesnt achieve an altitude of 20 degrees at any time from our shores, observers living in towns and cities will have to find a good observing spot with a flat horizon from the south-east around to the south-west if they dont want to spend the night dodging buildings and peeking between trees.

Jupiter culminates (reaching its highest point on the southern meridian) at about 1am BST around opposition: from London, it culminates at around +16.5 degrees altitude at 1.04am BST (12:04 UT); from Manchester, it peaks at between 14 and 15 degrees at 1.16am BST (12:16 UT); and in Edinburgh it reaches just over 12 degrees altitude at 1.20am BST (12:20 UT).

Jupiter will richly reward observers who have gone the extra mile to locate it, offering a generous-sized disc to enjoy, large enough indeed for even a humble pair of binoculars to resolve and for a small telescope to reveal its major bright zones and dark belts in its turbulent and ever-changing clouds tops.

The gas giants most famous individual feature is the Great Red Spot (GRS), a long-lived anticyclonic storm that has been raging in the planets South Tropical Zone (STrZ) for possibly 350 years. A telescope in the 150mm (six-inch) class should show the GRS at the times when it rotates into view (Astronomy Now has monthly listings of the GRSs appearances on the Jovian disc), along with a host of other transient features, such as white and dark ovals and festoons, but have a go with a smaller-aperture telescope if thats whats to hand.

On the night of 13/14 July, the GRS transits Jupiters central meridian at about 10.35pm BST (21:35 UT), but its barely 10 degrees up in the south-east at this time. However, it will remain visible for a couple of hours, as Jupiter climbs towards culmination, before it rotates out of view (Jupiter completes one rotation in just under ten hours). On 14/15 July, the GRS rotates into view at about 2.30am to 3am BST.

Jupiters low altitude from mid-northern latitudes makes observing it more problematic than normal, owing to the prevalence of turbulent seeing so close to the horizon. Atmospheric dispersion leads to noticeable colour effects, such as red and blue fringing on planets, caused by our atmosphere essentially acting as a prism. A red filter (Wratten 23/25) will help reduce dispersion fringing (though the latter filter has only 15 per cent transmission, so might be better employed with a moderate- to large-aperture telescope). An Atmospheric Dispersion Corrector (ADC) is a great accessory too.

A blue or light-blue filter (Wratten 80A/82A) will enhance the contrast between the planets dusky belts and bright zones, while the visibility of dark markings is enhanced by a yellow or orange filter (such as Wratten 12/21). The latter filter is an especially good choice for observing the GRS.

Jupiter is unique in the Solar System for its family of four large and bright Galilean moons: Io, Europa, Ganymede (the largest satellite in the Solar System, with a diameter of 5,268 kilometres [3,273 miles]) and Callisto. All can be seen through 10 x 50 binoculars. Following their eternal dance around their parent is a rewarding aspect of observing the giant planet, as they, together with their jet-black shadow, pass in front of the planet and at other times disappear behind and reappear from behind Jupiter (occultation) or move in and out of its massive shadow (eclipse).

The satellites move from east to west across the face of the planet and west to east behind it. After conjunction and before opposition, Jupiters shadow is cast to the west and shadow transits precedes transits, while eclipses happen before occultations. After opposition, the order is reversed.

Perhaps the most interesting of all the Galilean phenomena is watching the black shadows of the moons move across Jupiters face, though its much tougher to spot the moons themselves against the planets bright disc. A fascinating consequence of opposition is that a moon and its shadow can lie very close together, with occasionally the moon occulting its own shadow. On the night of 15/16 July, shortly after 3am BST (02:00 UT), Io and its shadow, seen very close together, will have just started a transit (see the graphic here). A 150mm telescope should be sufficient aperture to glimpse Ios shadow in any fleeting moments of steadier seeing.

As soon as Jupiter is observable on the night of 13/14 July, a pair of binoculars will show only three Galilean moons; Io and Europa lie roughly equidistant from the planet, to the east and west (left and right, through binoculars), respectively, while Callisto lies some way west of Jupiter. Ganymede is hidden behind the giant planet, after disappearing into Jupiters shadow at 9.36pm BST (20.36 UT). Its a shame that this event is not observable from UK shores, but Jupiter is barely above the horizon, having not long risen.

At this close to opposition (which occurs about 12 hours later), Jupiters giant shadow falls almost directly behind the planet, leaving an extremely thin sliver of shadow hugging the planets western (preceding) limb, which Ganymede gradually disappears into. See the graphic here showing the positions of the moons when Ganymede reappears at Jupiters eastern limb at around 1am. Obviously, the majority of eclipse events throughout the year occur when Jupiter is some way from opposition, so a moon will be seen to disappear in eclipse when it lies well away from Jupiters limb. Jupiters shadow falls increasing further westwards (or eastwards after opposition) from the limb the further the planet is from opposition.

On the following night, 14/15 July, all the moons will be visible for the entire night. Theres no end to the observational fun that can be had following Jupiters Galilean satellites. Astronomy Now has monthly listings of those Galilean moon events that are visible from UK shores.

Despite Jupiters less-than-ideal observing circumstances at this years opposition, theres still so much that can be seen by a determined observer. However, Jupiter is still a beautiful sight if all you want to do is gaze at it out of your window.

Our July issue features a complete guide to whats up in the night sky this month including how to observe Jupiter.Get your copy in the shops or order online for home delivery in print or digital download.

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Your best chance to see Jupiter this year - Astronomy Now Online

Popular UC San Diego astronomer Andy Friedman dies at 41 – The San Diego Union-Tribune

Andy Friedman, a UC San Diego astronomer known for his insights about supernovas and the expansion of the universe and for explaining them to the public in places like Astronomy magazine and San Diego Comic-Con, died on July 10 in San Diego. He was 41.

Friedman, who spoke with the joy and zest of Carl Sagan, one of his childhood heroes, succumbed to a rare form of cancer, according to his wife, Kristen Keerma Friedman.

He became the third prominent figure from UCSD to die in recent weeks. The campus also is mourning the loss of mathematician Ron Graham, whose work has been indispensable to the evolution of computing, and Flossie Wong-Staal, the virologist who co-discovered the cause of AIDS.

Friedman had suffered health problems over the years. But news of his death stunned friends and colleagues, including UCSD physicist Brian Keating, who recruited him to La Jolla, and physicist-science fiction author David Brin of Olivenhain.

The trio made up The Three Physicists, an informal group that periodically met to give public talks on science and philosophy.

Andy had opportunities to work with luminaries at other places, like MIT and Harvard, but he came here and we were so glad to have him, Keating said Monday.

He had a relentless curiosity, unparalleled mathematic ability, and a humanitarian soul. He could communicate with people, and his passion was infectious when he talked about things like quasars and the cosmos.

Brin said, Ive never known anybody who enjoyed a wider variety of ways to be alive. He was a scientist whose other interests extended to sculpture and painting and music and dabbling in science fiction. He had an epic rock and fossil collection. His passions included poking away at God by exploring the universe.

It is a trait of so many great American Jewish scientists, like Albert Einstein and Richard Feynman.

Friedman was born on April 7, 1979, at Mercy Hospital in San Diego. He was the son of a cardiologist and a producer of Jewish musicals.

He was raised in a home that loved science fiction and documentaries and books, said his wife, Kristen Keerma Friedman.

Her husband earned a bachelors degree in physics and astronomy at UC Berkeley and a doctorate in astronomy and astrophysics at Harvard. Friedman later went on to do research at MIT, working with renowned physicists David Kaiser and Alan Guth.

Friedman joined the UCSD research faculty in 2019, partly because of the opportunities in La Jolla and his desire to be close to his family.

His specialty was quantum mechanics, which is used to explain how the universe works at scales so small theyre hard to conceive, and supernova, an explosion known as the last hurrah of a star.

With Brin and Keating, he also dove into esoterica, tackling subjects such as the physics of free will.

Did you all come here today of your own free will or was your interest somehow programmed into the universe all the way back to the Big Bang? Friedman asked at the start of a talk in 2015.

I really do believe we have free will. So my approach is to ask, Do the laws of physics permit it? And if not, what ingredients might be missing?

His wife Kristen said Monday, He was never so happy as when he was speaking to the public. He thrived on it.

Friedman is survived by his wife, his parents, his wifes parents, as well as her sister.

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Popular UC San Diego astronomer Andy Friedman dies at 41 - The San Diego Union-Tribune

Astronomers Create Largest 3D Map of the Universe That Resolved a ‘Troublesome Gap’ About the Outer – Tech Times

Scientists revealed on Monday, July 20 the largest-ever 3D map of the universe.

In an AFP report,published by Yahoo News, hundreds of scientists from around 30 institutions across the globe worked on creating the 3D map. The project was launched more than two decades ago and studied more than four million galaxies.

Will Percival of the University of Waterloo in Ontario, Canada said the project created the "complete story of the expansion of the universe." Also, Percival said the scientists' work shows "the most accurate expansion history measurements" created on an extensive scale of time in space.

(Photo : Sloan Digital Sky Survey Team, NASA, NSF, DOE)Scientists revealed on July 20 the largest-ever 3D map of the universe.

It used the latest observations of the Sloan Digital Sky Survey (SDSS), which include data gathered after more than six years using an optical telescope in New Mexico.

Various galaxies and distance measurement studies also led to a better understanding of the expansion of the universe throughout billions of years.

The SDSS' recent study called the "extended Baryon Oscillation Spectroscopic Survey" (eBOSS) played an important role in creating the 3D map. Swiss Federal Institute of Technology (EPFL) Jean-Paul Kneib who initiated eBOSS in 2012, said the project aims to produce "the most complete 3D map of the Universe" during its lifespan.

While astrophysicists have already known that the Universe is expanding, they were not able to precisely measure the rate of expansion. However, with the 3D, they can reveal that the universe's expansion has started to accelerate and continue doing so.

This is due to the presence of dark energy, which follows Albert Einstein's general theory of relativity, although its origin is not yet completely known.

The eBOSS observations showed inconsistencies in the rate of expansion, as compared with past studies on the early universe.

The "Hubble constant," which is the currently accepted rate, is 10% slower than the value calculated from the distances between the neighboring galaxies.

(Photo : NASA Hubble Space Telescope)These Hubble Space Telescope images showcase 2 of the 19 galaxies analyzed in a project to improve the precision of the universe's expansion rate, a value known as the Hubble constant.

Meanwhile, the University of Utah scientists Kyle Dawson said the researchers have resolved a "troublesome gap" throughout 11 billion years after continuous observations for five years.

The 3D map reveals filaments of matter and voids that more precisely define the structure of the universe since it was only 380,000 years old. It is the first time researchers have illustrated space objects to show the distribution of matter in the universe.

Researchers observed the oldest and reddest galaxies to show the showing how the universe looks six billion years ago while they focused on the blue ones for more distant eras. Besides, they used quasars, which are galaxies with an extremely luminous supermassive black hole to illustrate the ancient universe.

In July 2019, the University of Hawaii's Institute of Astronomy unveiledCosmicflows, a set of 3D maps that illustrate the large structure of the universe. According toNBC News, Honolulu-based cosmologist Brent Truly revealed the fruit of his work for more than three decades.

The scale of Truly's work is so vast that shrink entire galaxies to dots, and blended the information like pixels on a computer screen. Tully said the master plan included four basic elements, including clusters, sheets, filaments, and voids."

Read also:NASA: Congratulations! You're Still a Gemini!

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Astronomers Create Largest 3D Map of the Universe That Resolved a 'Troublesome Gap' About the Outer - Tech Times

A nova, briefly visible in southern skies – EarthSky

A nova is a star that suddenly pops into view. Early stargazers thought they were new stars. Today, we know differently. Image via Ernesto Guido (@comets77 on Twitter).

Veteran comet hunter Robert McNaught from Coonabarabran, Australia, must have been perplexed and then surprised and then delighted when he noticed something peculiar on CCD images of the night sky, taken July 15, 2020. It was a faint, but visible star where none had appeared before. Such a star is called a nova, from a Latin word meaning new. This one is in front of the southern constellation Reticulum. Once confirmed by other astronomers, and reported in The Astronomers Telegram on July 16, the object was quickly announced to the worlds community of variable star observers as Nova Reticuli 2020 (N Ret 2020).

Its a rare find: a nova visible to the eye!

Astronomers have determined that this outburst is of the sort called a classical nova. That is, its created in a double-star system where one star is a white dwarf and the other is an ordinary main sequence star, not dissimilar from our sun. These two stars are close together in space, orbiting one another on a timescale of only hours. Because theyre close and because the white dwarf is a collapsed object with very powerful gravity (a teaspoon of white dwarf material would weigh several tons) hydrogen from the main sequence star is drawn into an accretion disk around the white dwarf. Eventually, this hydrogen piles onto the surface of the white dwarf. As explained on the website Cosmos from Swinburne University:

As more hydrogen (and helium) is accreted, the pressure and temperature at the bottom of this surface layer increase until sufficient to trigger nuclear fusion reactions [the same process that causes our sun and most other stars to shine]. These reactions rapidly convert the hydrogen into heavier elements creating a runaway thermonuclear reaction where the energy released by the hydrogen burning increases the temperature, which in turn drives up the rate of hydrogen burning.

The energy released through this process ejects the majority of the unburnt hydrogen from the surface of the star in a shell of material moving at speeds of up to 1,500 km/s. This produces a bright but short-lived burst of light the nova.

A classical nova outburst can occur again and again in a system of this kind.

Nova Reticulum 2020 is associated with a known object in the database of the American Association of Variable Star Observers, labeled MGAB-V207 and categorized as a cataclysmic variable star. These sorts of stars are known to undergo classical nova outbursts due to mass transfer between a main sequence star and a white dwarf.

In a classical nova, a dense white dwarf pulls material from a companion star. The material piles up on the white dwarfs surface until thermonuclear processes begin, creating an outburst. Image via NASA/ JPL-Caltech.

Can you see Nova Reticuli 2020? Possibly, if it hasnt faded yet, and if you live in the Southern Hemisphere, where the constellation Reticulum can be seen. On July 17, writing at Astronomy.com, Alison Klesman said Nova Reticuli 2020 was shining at around magnitude 5.

That is, its visible to the eye, but only barely.

If its still visible to the eye, you will need a very dark to see the nova. If you have that and a constellation chart to show you how to find Reticulum look first for the bright stars Alpha and Gamma Doradus, shown on the chart below (apologies for the blurriness of the chart; be sure to view it larger).

Good luck!

View larger. | If you live in the Southern Hemipshere, you can see the constellation Reticulum and the nova. You can pinpoint Nova Reticuli 2020 by looking roughly 5 degrees west of magnitude 3.3 Alpha Doradus and 4.25 degrees southwest of magnitude 4.3 Gamma Doradus. Notice that these 2 stars make a triangle with the nova. If the nova has gotten fainter, try using binoculars to bring it into view. Image via Alison Klesman/ Astronomy.com.

Congratulations to comet hunter Robert McNaught, who was the first to spot Nova Reticuli 2020! Image via Abc.net.au.

Bottom line: Astronomers have spotted a classical nova outburst in a type of variable star that involves a white dwarf orbiting a main sequence star. Nova Reticulum 2020 has been briefly visible from the Southern Hemisphere. At this writing, we do not know if it is still visible.

Via The Astronomers Telegram

Via the American Association of Variable Star Observers

Via Astronomy.com

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A nova, briefly visible in southern skies - EarthSky

Enjoy the Stars in the Astronomy Photographer of the Year Shortlist – My Modern Met

Statue of Liberty Nebula by Martin Pugh (Australia). Shortlist, Stars & Nebulae.Photographed using narrowband filters to accentuate the energy levels occurring in each emission line, sulfur was mapped to red, hydrogen to green and oxygen to blue. An additional 4 hours per RGB channel were acquired and substituted into the image, particularly for the stars. While aptly titled the Statue of Liberty Nebula (NGC 3576), the irony is that this is a southern hemisphere object. At lower left in the image is NGC 3603 containing the Starburst Cluster. NGC 3576 is located in the Carina arm of the Milky Way at approximately 20,000 light-years distant.

Moved by the beauty of the stars, astrophotographers from around the world submitted their best work to the annual Insight Investment Astronomy Photographer of the Year contest. Run by Royal Observatory Greenwich each year, the competition is the place to view the artistry found in our sky. Thousands of photographs were submitted across 11 categories and, now, the 2020 shortlist has been revealed.

Now in its 12th year, the contest attracted photographers from 70 different countries who collectively entered over 5,200 images. The high quality of the shortlist means that the judges will have their hands full this year. From vibrant photos of the Northern Lights to faraway nebulae to incredible photos of our Sun, the list shows the wide spectrum of astrophotography.

Astronomy is one of the most accessible sciences and everyone has looked up at the night sky at one time or another and wondered what is out there in the cosmos, says competition judge and Royal ObservatoryGreenwich Astronomer, Dr. Emily Drabek-Maunder. Astrophotography bridges the gap between art and science, highlighting the natural beauty of our Universe. The goal of the Insight Investment Astronomy Photographer of the Year competition is to use these powerful photographs of space to engage the public with the big questions science is trying to answer, from the inner workings of a galaxy to how our Solar System came to be.

This years contest also features two special awards. The Annie Maunder Prize for Image Innovation celebrates photos created using publicly available images. Entrants have been asked to process and manipulate the raw data to create something of their own. The other new award is the Sir Patrick Moore Prize for Best Newcomer. This prize goes to people who have just started their journey into astrophotography during the last year and consider it a hobby. And to prove that one doesnt need to have fancy equipment to take a good photo, special consideration will be given to those who use an inexpensive starter kit.

The winners of the Insight Investment Astronomy Photographer of the Year contest will be announced on September 10, 2020. The overall winner will receive 10,000 (about $12,529) and category winners will take home 1,500 (approx. $1,880). All winners and shortlisted entries will be featured in a special exhibition at the National Maritime Museum starting in October 2020.

M16 by Alexios Theodorov (Russia). Shortlist, Annie Maunder Prize for Image Innovation.This entry tries to catch the feel of stargazing through basic optical instrumenta kind of Galileos telescope. Special processing of the image includes converting to Lab, channel mixing, increasing contrast, and applying filters, with the aim of illustrating that images with limited color range may be as stunning as full-color ones.

Northern Dragons Eye by Elena Pakhalyuk (Ukraine). Shortlist, Aurorae.The photographer loves to travel, especially exploring the north and chasing the Northern Lights. Trying to capture how ordinary things can take magical forms under the lights, the photographer selected and lit this rocky outcrop and waited for the aurora to work its magic.

Eruption. by Elena Pakhalyuk (Ukraine). Shortlist, Our Sun.The photographer was inspired to imagine what the Crimean peninsula would look like in the distant past, when thousands of volcanoes erupted on Earth. She used lighting and long exposure to illustrate this. The resulting image sees everything combined into one large panorama image and processed in a photo editor.

Solar System Through my Telescope by Vinicius Martins (Brazil). Shortlist, Best Newcomer.This image is a composition that the photographer made using their best images of the solar system. The individual images were taken between July 2019 and February 2020. All images were obtained using the same planetary imaging method and combined.

The Red Lake of Stars by Bryony Richards (USA). Shortlist, Skyscapes.Years ago, before over-fishing, Little Redfish Lake was called as such due to the vast numbers of salmon turning the lake a red color. The red coloration is no longer seen because of salmon, but the color of sunsets and airglow during the night still turn the waters a vibrant red. It is these beautiful warm echoes of red, combined with the mirror-like reflections of the Sawtooth Mountains in the distance and the alignment of the Milky Way with the mountains that make Little Redfish Lake one of the most spectacular places the photographer has ever shot at night. The photographer recalls that we were fortunate enough that night to have the lakeshore to ourselves, just three of us, and a rather excited dog who tried his best not to run into our tripods! We spent the sunset here, waiting for the stars to come out and the Milky Way core to rise, marveling at the red color of the water.'

M33: The Triangulum Galaxy by Rui Liao (China). Shortlist, Galaxies.This sharp image shows off M33s blue star clusters and pinkish star forming regions along the galaxys loosely wound spiral arms. In order to depict these star-forming regions, the photographer has taken a total of 26.5 hours of exposure time. For the photographer, the enjoyment comes in gazing at the red flowers in the image, mingled in blue star clusters, and the satisfaction that his efforts paid off.

Kynance Cove under the Milky Way by Louise Jones (UK). Shortlist, Best Newcomer.This image is only the photographers second attempt at shooting the Milky Way. It shows our galaxy over Kynance Cove in Cornwall, a beautiful spot with dark skis. It was taken on a cold, but fabulous night under the stars. As it was July, the sky was very blue, with full darkness only for about an hour. The foreground was taken at dusk and the sky is a stack of 4 images of 25 seconds taken later when the Milky Way appeared, the sky and foreground blended together in post-processing.

Stokksnes Aurora by Ben Bush (UK). Shortlist, Aurorae.This image captures the stunning Stokksnes looking to the Vestrahorn and the most powerful and beautiful night of aurora the photographer had ever seen. He traveled 1250 miles to try and capture his dream. In order to get the shot, the photographer ended up knee-deep in the North Atlantic in -6 degrees Celsius. The challenge was to capture the reflections in the water, on the black sand beach, and also not to over-expose the aurora. The photographer describes this as a truly awe-inspiring experience and one he feels blessed to have witnessed and captured on camera.

39% Crescent Moon by Richard Addis (UK). Shortlist, Our Moon.This image of the Moon at 39% illumination was captured through eleven videos of different areas, which were stacked and then stitched together. The saturation process revealed the mineral compositions in the Lunar Basalts on the surface. These vivid browns and blues are due to high concentrations of titanium and iron. The photographer loves the contrast along the terminator and the close-up detail and clarity of this image.

Beautiful Persian Gulf Nights by Mohammad Sadegh Hayati (Iran). Shortlist, People & Space.On one of the many hiking trails along the coastline, the photographer discovered this incredible lookout. The scale of the vista encouraged the photographer to capture a 360-degree panoramic image of the entire sky using 60 15-second exposures. The movement of the clouds meant that the photographer had a short time to capture the Milky Way. The photographer is pictured, enjoying the wonderland he stumbled across.

The Bat Nebula by Josep Drudis (USA). Shortlist, Stars & Nebulae.When a massive star explodes as a supernova it expels enormous amounts of materials, leaving behind one of the most beautiful examples of nebulae. This is the origin of the Veil Nebula, a large gas cloud in the constellation Cygnus, the Swan. This image shows just a small fragment of this nebula. The beauty and fine detail of the interlaced wisps of oxygen, nitrogen, and hydrogen, here mapped to their natural colors, is awe-inspiring. In this image, we can admire one of the life-building processes in the Universe.

Stargazing Giant by Dai Jianfeng (China). Shortlist, People & Space.This image is the view of the Milky Way rising above the Moai at Ahu Akivi. Ahu Akivi is a particularly sacred place in Easter Island in the Valparaso Region of Chile, looking out towards the South Pacific Ocean. The site has seven moai, all of equal shape and size, and is also known as a celestial observatory that was set up around the 16th century. The shot highlights the central bulge of the Milky Way, the constellation Scorpio, as well as the planets Jupiter and Saturn.

Total Solar Eclipse, Venus and the Red Giant Betelgeuse by Sebastian Voltmer (Germany). Shortlist, Our Sun.The 50th Anniversary of ESOs La Silla Observatory culminated with a breath-taking and very clear Total Solar Eclipse. In a very long process, the photographer calibrated, aligned, and stacked 96 frames together, revealing the streamers and the faint corona. Stars also became visible, especially the red giant Betelgeuse (left) which started dimming in the months after. For the different star brightnesses of the tiny star dots the photographer used his action set RealStars; so he was able to show the brightness of Betelgeuse in comparison to Bellatrix and the other stars during daytime.

Something Old, Something New by Jay Evans (Austraila). Shortlist, Skyscape.The incredible site of the old Lithgow Blast Furnace has been restored as a heritage icon in the area reflecting on the past history of the beginnings of the iron and steel industries in Australia. With some prior planning, visiting at night provides the mesmerizing opportunity to capture the Galactic Core in the Milky Way as it passes overhead. The photographer took this opportunity to try out the first Astro shots captured using a new high megapixel camera, yet to be released.

The Moon and the Shard by Mathew Browne (UK). Shortlist, Our Moon.After three failed attempts, the photographer finally got to shoot an image of Londons iconic Shard skyscraper with a full moon behind it. The moon races through frame meaning the photographer only had a few minutes to capture the shot.

NGC 2442 in Volans by Martin Pugh (Australia). Shortlist, Galaxies.The photographer was particularly excited to capture this image, having relocated his CDK17 to Chile in May 2019. He found that the acquired data was of spectacular quality and given the seemingly endless clear nights at that location, he was able to accumulate a great deal in a relatively short period of time. The photographer captured 3 hours of hydrogen and it was enough to accentuate the star birth regions occurring in the galaxy.

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Enjoy the Stars in the Astronomy Photographer of the Year Shortlist - My Modern Met

The Sky This Week: Comet NEOWISE appears at sunset – Astronomy Magazine

Monday, July 20New Moon occurs at 1:33 P.M. EDT.

Saturn reaches at opposition at 6 P.M. EDT, when it will lie 836 million miles (1.35 billion kilometers) from Earth. As soon as the Sun sets, the ringed planet is rising in the southeast, with Jupiter about 7 to its west. Saturn glows at an easy magnitude 0.1 for observers without optical aid, but binoculars or a telescope will bring into view its stunning rings. They stretch nearly 42" across, more than twice the diameter of the planets 19"-wide disk. As full darkness falls, see if you can spot the rings dark Cassini Division or the planets bright moon Titan, nearly 3' east of Saturns center.

Saturn lies in the constellation Sagittarius, and the region around it is rich with additional observing targets tonight. These include Jupiter, Pluto, and the globular clusters M55 and M75. With no Moon to create glare, these and other faint objects should be easier to spot and appear grander against the dark-sky backdrop.

Tuesday, July 21Summertime is the best time to try spotting noctilucent, or night-shining, clouds. These wispy, eerie clouds hang high in Earths atmosphere about 50 miles (80 km) above the surface, far higher than the lower atmosphere where other clouds and weather occur. Noctilucent clouds comprise ice crystals that form on dust grains high in the atmosphere, which are then illuminated by the Sun. Because of their height, these clouds can reflect light long after the Sun has set (or before it rises) from an observers location.

Wednesday, July 22The Southern Delta Aquariid meteor shower is now ramping up for its peak on July 29, when observers can expect about 20 shower meteors per hour. In fact, the shower has been active most of the month, officially starting on the 12th. As the date of the peak approaches, you may notice more and more sporadic meteors in the sky, particularly if you observe for long periods of time from a dark site. The showers radiant in Aquarius the Water-bearer rises late in the evening and is visible all morning until sunrise, climbing higher in the sky. To find it, locate bright Jupiter and Saturn, then scan about 35 east of a point roughly between the two planets. With New Moon now past, the next several days are an ideal time to watch for meteors. The best time to look is early morning, before dawn starts to brighten the sky.

Mercury is at greatest western elongation (20) at 11 A.M. EDT.

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The Sky This Week: Comet NEOWISE appears at sunset - Astronomy Magazine

Powerful eruptions on the Sun might trigger earthquakes – Astronomy Magazine

Through decades of research, scientists have learned that large, powerful earthquakes commonly occur in groups, not in random patterns. But exactly why has so far remained a mystery. Now, new research, published July 13 in Scientific Reviews, asserts the first strong though still disputed evidence that powerful eruptions on the Sun can trigger mass earthquake events on Earth.

To the unaided eye, the Sun might seem relatively docile. But our star is constantly bombarding the solar system with vast amounts of energy and particles in the form of the solar wind. Sometimes, however, formidable eruptions on the Suns surface cause coronal mass ejections, or especially energetic floods of particles including ions and electrons that careen through the solar system at breakneck speeds. When they reach Earth, these charged particles can interfere with satellites, and under extreme circumstances, take down power grids. The new research suggests that particles from powerful eruptions like this specifically, the positively charged ions might be responsible for triggering groups of strong earthquakes.

Earthquakes typically occur when rocks grind past one another as Earths tectonic plates shift and jostle for position. When the intense friction thats locking plates together is overcome, the rocks break, releasing tremendous amounts of energy and shaking the ground.

But scientists have also noticed a pattern in some large earthquakes around the planet: they tend to occur in groups, not at random. This suggests there may be some global phenomenon thats triggering these worldwide earthquake parties. And though many researchers have done statistical studies to try to determine a cause before, no compelling theories have yet been rigorously proven.

So, to tackle the lingering mystery, the researchers of this latest study combed through 20 years of data on both earthquakes and solar activity, searching for any possible correlations. Specifically, the team used data from NASA-ESAs Solar and Heliospheric Observatory (SOHO) satellite, compiling measurements of protons (positively charged particles) that come from the Sun and wash over our planet.

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Powerful eruptions on the Sun might trigger earthquakes - Astronomy Magazine

Astronomy Photographer Of The Year 2020 Shortlisted Images Selected – ePHOTOzine

The Red Lake of Stars Bryony Richards (USA)

Once again, the Royal Observatorys 'Insight Investment Astronomy Photographer of the Year 2020' has received thousands of outstanding images.

Entrants have captured wonders from across our solar system, galaxy and the wider Universe; from the second-largest planet in our solar system, Saturn, which is wreathed by a complex system of icy rings and surrounded by more than 60 moons; an Eruption on our suns surface, a prominence on one of the stars most active regions; to the Sculptor Galaxy that was discovered by Caroline Herschel in 1783 and known as a starburst galaxy for its intense star formation regions.

The Moon and the Shard Mathew Browne (UK)

Shortlisted images from this years entrants also include a Full Moon illuminating the jagged peak of The Shard, London, a mesmerising aurora over Stokksnes headland on the Icelandic coast and a remarkable scene of a total solar eclipse, the planet Venus and the star Betelgeuse, captured at ESOs La Silla ESO Observatory, in the Atacama Desert, Chile.

Cold Night on the Yellowstone Jake Mosher (USA)

The competition, run by the Royal Observatory Greenwich, sponsored by Insight Investment and in association with BBC Sky at Night Magazine, is now in its twelfth year and has broken the record number of entries once more, receiving over 5,200 entries from enthusiastic amateurs and professional photographers, taken from almost 70 countries across the globe.

Something Old, Something New Jay Evans (Australia)

Competition judge and Royal Observatory Greenwich Astronomer, Dr Emily Drabek-Maunder said of the competition: "Astronomy is one of the most accessible sciences and everyone has looked up at the night sky at one time or another and wondered what is out there in the cosmos. Astrophotography bridges the gap between art and science, highlighting the natural beauty of our Universe. The goal of the Insight Investment Astronomy Photographer of the Year competition is to use these powerful photographs of space to engage the public with the big questions science is trying to answer, from the inner workings of a galaxy to how our Solar System came to be."

The Cave of the Wild Horses Bryony Richards (USA)

The competitions judges also include renowned comedian and keen amateur astronomer, Jon Culshaw; Art Editor of BBC Sky at Night Magazine Steve Marsh and a host of experts from the worlds of art and astronomy. The winners of the competitions nine categories and two special prizes will be announced on Thursday 10 September 2020. The winning images will be displayed in an exhibition at the National Maritime Museum, alongside a selection of exceptional shortlisted images. Winners and shortlisted entries will also be published in the competitions official book, available in September from bookstores and online, and to pre-order from the Royal Museums Greenwich online shop.

For more information, visit thecompetition website.

Galactic Portal Marcin Zajac (USA)

To see last year's winners have a read of these features:Stunning Astronomy Photographer Of The Year 2019 Winning Images Announced & Astronomy Photographer Of The Year 2019 'People's Choice' Revealed

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Astronomy Photographer Of The Year 2020 Shortlisted Images Selected - ePHOTOzine

Astronomy Photographer of the Year 2020 Shortlist Revealed – PetaPixel

The Royal Observatorys prestigious Astronomy Photographer of the Year 2020 competition has revealed the shortlisted photos from this years entries.

A record-breaking 5,200 entries shot by amateur and professional photographers located in nearly 70 countries were received this year by the Insight Investment Astronomy Photographer of the Year 2020 contest.

Here are the shortlisted photos in each of the major categories:

Produced using publicly available images. Entrants must process and manipulate the raw data in order to create a new version of that image.

Photographs featuring auroral activity.

Deep space objects beyond the Milky Way galaxy, including galaxies, galaxy clusters, and stellar associations.

Lunar images including lunar eclipses and occultation of planets.

Solar images including solar eclipses and transits.

Photographs of the night sky including people or a human interest element.

Landscape and cityscape images of twilight and the night sky featuring the Milky Way, star trails, meteor showers, comets, conjunctions, constellation rises, halos and noctilucent clouds alongside elements of earthly scenery.

Deep space objects within the Milky Way galaxy, including stars, star clusters, supernova remnants, nebulae and other intergalactic phenomena.

Pictures taken by budding astronomers under the age of 16 years old.

The winners of this years contest will be announced on September 10th, 2020, and the photos will be exhibited in the National Maritime Museum from October 2020.

The overall winner of this years competition will walk home with 10,000 (~$12,600) while winners in the other categories will be awarded 1,500 (~$1,900).

You can view last years winning images over on the competitions website.

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Astronomy Photographer of the Year 2020 Shortlist Revealed - PetaPixel

See Jupiter and Saturn at their brightest this week – Space.com

Planets are very much in the fore these days, especially with the two largest Jupiter and Saturn now putting on a show as prominent evening luminaries. This week, both planets appear at their very best, with Jupiter having just arrived at opposition this past Tuesday (July 14) and Saturn to reach its own opposition on Monday (July 20).

On Dec. 21, these two planets will be in conjunction meaning they'll share the same celestial longitude while making a close approach in the night sky for the first time since the year 2000. It takes Saturn almost 30 years to make one trip around the sun, while it only takes Jupiter about 12 years to complete one solar revolution. As a result, Jupiter appears to overhaul Saturn at intervals of roughly 20 years.

Let's check out both of these giant worlds, which will remain prominent objects in our evening sky through the balance of this year. Saturn and Jupiter provide telescope users with a feast of features. Saturn of course has its splendid ring system and Jupiter can boast a restless atmosphere and retinue of bright moons.

Related: The brightest planets in July's night sky

As we just noted, Jupiter arrived at that point in the sky directly opposite to the sun, called "opposition," on Tuesday (July 14). If the planets' paths around the sun were true circles, this would also coincide with Earth's closest approach to Jupiter, 384.8 million miles (619.1 million kilometers). However, because the planets' orbits are slightly oblong, that actually occurred the following day, on Wednesday (July 15).

Opposition occurs when the Earth, moving faster in its orbit than Jupiter, overtakes it. (This is true for any of the outer planets.) From now on, we'll leave Jupiter behind, catching up with the planet again on Aug. 19, 2021. Jupiter is also currently moving closer to the sun in its own elliptical path and will reach its closest point to the sun, 460 million miles (740 million km), at its perihelion point on Jan. 20, 2023.

Jupiter, the largest planet in the solar system, shines as a brilliant silvery "star" to the upper left of the famous Teapot asterism of Sagittarius, low in the east-southeast sky as dusk arrives and will now appear to climb higher in the evening sky in the weeks to come.

Currently, this giant planet is ready for telescopic observing by 10:45 p.m. local time, when it will stand roughly one-quarter of the way up from the horizon to the point directly overhead, called the zenith. It reaches its highest position in the south around 12:30 a.m. and is heading toward its setting in the west-southwest during dawn.

With a diameter of 88,800 miles (143,000 km), Jupiter is a colossal ball of hydrogen and helium without a solid surface. It has a rocky core encased in a thick mantle of metallic hydrogen enveloped in a massive atmospheric cloak of multi-colored clouds of ammonium hydrosulphide.

In a strange sense, Jupiter might even be referred to as a "stillborn star," for it has the makings (mostly hydrogen) if not the mass of a stellar body. Its relative smallness, however, prevents the initiation of the nuclear processes that could have turned it into a full-fledged star. Had this been the case, we would have the distinction of living within a binary star system.

Jupiter is the most consistently interesting object in the solar system after the moon and the sun and has always held a special place in the hearts of telescope viewers.

The smallest telescope even steadily held 7-power binoculars show Jupiter as a tiny disc, while a medium-size telescope reveals numerous dark belts, light zones and a wealth of festoons, garlands, ovals and other features extending here and there.

But Jupiter's greatest telescopic treasure are its four Galilean satellites that run a merry chase with each other around the planet (in all Jupiter has 79 confirmed moons), changing their respective positions from hour to hour and night to night.

Typically, at least two or three Galilean moons are visible at any given moment. The four Io (I), Europa (II), Ganymede (III) and Callisto (IV), numbered by the order in which they were named are all larger than Earth's moon. They can be followed for hours as they speed in front of Jupiter (throwing their shadows on the planet), vanish behind its giant disk or plunge into its shadow. They appear as tiny stars nearly in line and changing their places in the line as they revolve around the planet in orbits nearly edgewise to us.

On July 22, for example, we would see all four satellites on one side of Jupiter. Moving outward from Jupiter, they will also be, interestingly, in numerical order: Io, Europa, Ganymede and Callisto.

Now is also the best time to observe the telescopic showpiece of the night sky, the ringed planet Saturn. Saturn, like Jupiter, also currently lies in the constellation of Sagittarius, the archer, adjacent to the border of another zodiacal constellation, Capricornus, the sea goat.

On Monday night (July 20) Saturn arrives at its own opposition, when it too will lie on the opposite side of the sky from the sun. This is also when its apparent size is greatest, and it puts on an all-night performance with greatest gleam. It is now shining at magnitude +0.1, just a trifle dimmer than Vega, the brightest star of the Summer Triangle, yet still only about 8% as bright as nearby Jupiter. (Magnitude is a measure of brightness used by astronomers, with smaller numbers indicating brighter objects.)

In ancient days, before we had knowledge of the more distant planets Uranus and Neptune, Saturn was presumed to be the farthest and slowest-moving known planet. In mythology, Saturn closely resembled the Greek god Cronus, but he's more usually recognized as the Roman god of agriculture. The name is related to both the noun satus (seed corn) and the verb serere (to sow).

So, why would the planet Saturn be linked to agriculture? Perhaps a clue can be found from the ancient Assyrians who referred to Saturn as lubadsagush, which translated meant "oldest of the old sheep." Possibly this name was applied because Saturn seems to move so very slowly among the stars; it may have also reminded skywatchers of the slow gait of plowing oxen or cattle.

Seen with only the naked eye, Saturn now appears a very bright yellow-white star shining with a steady glow, but the ring system that makes it both beautiful and spectacular cannot be seen. Any small telescope magnifying more than 30 power, however, will clearly show the rings. They consist of countless billions of particles largely water ice that range in size from microscopic specks to flying mountains miles across. Each particle revolves around Saturn in its own orbit. They are likely the pulverized icy fragments of a satellite that probably ventured too close to Saturn and was torn apart by tidal forces.

Currently, the rings are dramatically tipped nearly 22 degrees to our line of sight. When Galileo Galilei's crude, imperfect "optick tube" revealed Saturn as having an odd pair of appendages or smaller companion bodies on either side, leaving him completely baffled. He announced this discovery in 1610 with an anagram written in Latin. The jumbled letters could be transposed to read: Altissimum planetam tergeminum observavi ("I have observed the highest planet to be triple").

Later, when the rings turned edgewise to Earth and the two companions disappeared, Galileo invoked an ancient myth when he wrote, "Has Saturn swallowed his children?" It was not until March 25, 1655 that a Dutch mathematician, Christiaan Huygens, utilized a much better telescope, and saw the rings for what they really were. Huygens also discovered Saturn's largest moon, Titan, larger than either Mercury or our moon. It is but one of 82 known satellites circling Saturn.

The theoretical construction of Saturn 74,900 miles (120,500 km) wide resembles that of Jupiter; it is either all gas, or has a small dense center surrounded by a layer of liquid and a deep atmosphere. And since its specific gravity is less than that of water, Saturn would float if you could find an ocean large enough to drop it in!

One of my astronomy mentors, Kenneth L. Franklin (1923-2007), former chief astronomer at New York's Hayden Planetarium would periodically make reference to our "dynamic and ever-changing sky." Such an eloquent description certainly will fit the evening sky on Aug. 1, as we'll have a celestial summit meeting of sorts taking place in southeast sky at nightfall. A waxing gibbous moon will be accompanied by Jupiter, hovering above it, while Saturn will be well off to the moon's left.

If you have a telescope, why not invite some friends and neighbors over that evening? First give them a look at the moon. Then, without revealing what it is, train your scope on that bright yellow-white "star" to its left and tell them to take a look. You'll likely hear exclamations of delight, especially if they're getting their first look at the ringed planet!

Joe Rao serves as an instructor and guest lecturer at New York'sHayden Planetarium. He writes about astronomy forNatural History magazine, theFarmers' Almanacand other publications. Follow uson Twitter@Spacedotcomand onFacebook.

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See Jupiter and Saturn at their brightest this week - Space.com

‘Partial supernova’ blasts white dwarf star across the Milky Way – Space.com

A strange white dwarf star hurtling through the Milky Way may be the survivor of a "partial supernova," a new study finds.

White dwarfs are the cool, dim Earth-size cores of dead stars that are left behind after average-size stars have exhausted their fuel and shed their outer layers. Our sun will one day become a white dwarf, as will more than 90% of the stars in the Milky Way.

Previous research found that white dwarfs usually have internal structures arranged in layers. Their cores are mostly carbon and oxygen, which is usually surrounded by a layer of helium and then a layer of hydrogen. Astronomers examining white dwarfs usually see just hydrogen, just helium or sometimes a mix of helium and carbon (although there are exceptions that hint at unusual pasts.)

Related: To find alien life, we should focus on white dwarf stars

In a new study, scientists zeroed in on the white dwarf SDSS J1240+6710, located about 1,430 light-years from Earth. Discovered in 2015, prior work found this white dwarf had an unusual atmosphere that seemed to possess neither hydrogen or helium, but instead was composed of a weird mix of oxygen, neon, magnesium and silicon.

Researchers in this new study used the Hubble Space Telescope to take a closer look at the white dwarf and they identified carbon, sodium and aluminum in the object's atmosphere. This mix sets this white dwarf apart from any other previously known, they said.

In this study, the scientists also found that the white dwarf was traveling about 560,000 miles per hour (900,000 kilometers per hour) in the opposite direction of the way the galaxy is rotating. Moreover, it had an especially low mass for a white dwarf only about 40% the mass of our sun.

"When we found this unusual white dwarf was really low in mass and really moving fast, that really triggered my curiosity into what happened to it in its past," study lead author Boris Gnsicke, an astrophysicist at the University of Warwick in England, told Space.com.

What might explain all these strange details about this white dwarf? The researchers in this study think that a thermonuclear explosion didn't completely destroy the white dwarf but, rather, a "partial supernova" blasted what remained of the object across the Milky Way.

Supernovas are the most powerful star explosions in the universe, bright enough to momentarily outshine entire galaxies. They can occur when a white dwarf dies from siphoning off too much mass from a companion star. All the extra weight from the stolen mass squeezes the white dwarf's core, which drives the core's temperature and density high enough to set off a thermonuclear chain reaction that explosively obliterates the white dwarf.

In the case of SDSS J1240+6710, the scientists noted the elements seen in the white dwarf's atmosphere could have all been produced in the first thermonuclear reactions of a supernova. However, there is a clear absence of what is known as the iron group of elements iron, nickel, chromium and manganese.

These heavier elements are normally cooked up from lighter elements, and their absence in this white dwarf suggests it only went part of the way through a supernova, failing to reach the high temperatures and densities needed to forge iron-group elements.

"That's what makes this white dwarf unique it did undergo nuclear burning, but stopped before it got to iron," Gnsicke said. "When it had its supernova event, it was likely just brief, maybe a couple of hours."

The researchers suggested that SDSS J1240+6710 was small compared to white dwarfs that normally undergo thermonuclear supernovas. As such, only a miniature supernova may have occurred, a type Iax, a partial supernova weak enough to leave behind most of a white dwarf.

"In the old days, researchers would have thought a thermonuclear supernova would destroy a white dwarf entirely, but in the past 10 or 15 years, scientists have found it's possible that a partial supernova could happen that leaves part of the white dwarf behind, burned and charred," Gnsicke said. "The explosion isn't powerful enough to totally disrupt the star."

This explosion would have blasted SDSS J1240+6710 away from its companion, ripping matter off the small white dwarf and hurling it through deep space at the speed at which it orbited its partner, Gnsicke said. This scenario would help to explain the white dwarf's speed, puny size and bizarre atmosphere.

Based on SDSS J1240+6710's mass and temperature, the scientists estimated this partial supernova occurred about 40 million years ago. Much remains unknown about the white dwarf's companion, but the researchers think it could have been a white dwarf much like SDSS J1240+6710.

Previous research into the origins of thermonuclear supernovas largely focused on larger white dwarfs. Now that this new study suggests that smaller white dwarfs can undergo similar explosions, future models could explore how these outbursts and their subsequent remnants might look, Gnsicke said.

"Thanks to the Gaia space mission, which was able to identify more than 50,000 white dwarf candidates, we can examine these white dwarfs to get a much better idea of what happens during these types of partial supernovas, such as what are the products of burning," Gnsicke said. "Hopefully we'll be able to identify a few dozen similar systems. We can start to go from one weird outlier to a small class of systems."

Future research could also explore whether astronomers may have already detected the brief dim flashes of light Gnsicke and his colleagues suspect are linked with this kind of strange white dwarf.

"It will be interesting to see if they will be able to find these very short supernova-like events that likely were just dismissed until now because they didn't look like supernovae," Gnsicke said. "Since they were so short, the chances were very slim to catch one, and there was very little time to follow up on whether any such detection was real. But in principle, the data suggesting these events are real exists somewhere."

The scientists detailed their findings online July 15 in the journal Monthly Notices of the Royal Astronomical Society.

Follow Charles Q. Choi on Twitter @cqchoi. Follow us on Twitter @Spacedotcom and on Facebook.

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'Partial supernova' blasts white dwarf star across the Milky Way - Space.com

Moon may be 85 million years younger than astronomers think it is, new study suggests – Firstpost

FP TrendingJul 17, 2020 08:39:19 IST

A new study now suggests that Earth's satellite is about 85 million years younger than earlier.

According to a report in Science Alert, researchers say lunar rock samples collected on the Apollo missions are not old enough to verify the normally accepted thought that the Moon is 4.51 billion years old.

Earth's natural satellite was formed from debris created by a collision between the young Earth and a protoplanet. Image credit: Ron Miller

As per the report, the commonly accepted hypothesis is that the Moon was formed from the debris of a collision between the Earth and a smaller planet called Theia. The collision led to the spewing out of molten rock that eventually cooled down and solidified into one whole body that began orbiting the Earth.

This means that the rock that makes up the Moon came from Earth and can be used to date it. Now study now suggests that the Moon was created when the Earth was almost fully formed.

Space.com reported that researchers at the German Aerospace Center found out that, not only did the moon once have a massive, fiery magma ocean, but our rocky satellite also formed later than scientists previously expected.

According to new research, the moon's birth has been pegged at only 4.425 billion years ago.

One of the oldest Moon rocks Image credit: NASA

The research team used mathematical models to calculate the composition of the moon over time. Basing their research on the idea that the moon was host to a massive magma ocean, researchers calculated how minerals that formed as the magma cooled and solidified over time.

As per a statement issued by study co-author Sabrina Schwinger, a researcher at the German Aerospace Center, "By comparing the measured composition of the moon's rocks with the predicted composition of the magma ocean from our model, we were able to trace the evolution of the ocean back to its starting point, the time at which the moon was formed."

Thorsten Kleine, a professor at the Institute of Planetology at the University of Mnster in Germany added that this is the first time that the age of the moon can be directly linked to an event that occurred at the very end of the Earth's formation.

These findings were published in the journal of Science Advances.

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Moon may be 85 million years younger than astronomers think it is, new study suggests - Firstpost

Astronomers Spot Strange Space Object, Have No Idea What It Is – Popular Mechanics

An international team of astronomers claims to have discovered a new type of celestial object.

Scientists first spotted the objects, which they've dubbed "Odd Radio Circles" (ORCs), in the heaps of data that were collected during a preliminary survey by the Australian Square Kilometre Array Pathfinder's Evolutionary Map of the Universe project, reports Live Science. The ORCs are mostly circular (one is shaped like a disc) and three of them are brighter around the edges.

The mysterious objects can only be spotted with radio telescopes. They're completely invisible to X-ray, optical and infrared telescopes. What's more, they "do not seem to correspond to any known type of object," the researchers write in their paper, which was published on the preprint website, arXiv.

"Circular features are well-known in radio astronomical images, and usually represent a spherical object such as a supernova remnant, a planetary nebula, a circumstellar shell, or a face-on disc such as a protoplanetary disc or a star-forming galaxy," the researchers write.

Norris et. al, 2020

The team combed through other sources of data to see if they could spot anything similar. That's when they found the fourth circle, tucked away in data gathered in 2013 by the Giant MetreWave Radio Telescope in India. The ORCs have been spotted in data from other radio telescopes around the world, ruling out the possibility that a telescopic glitch could have caused the readings.

So what could these strange sightings be?

In their paper, the team runs through a list of scenarios that could account for the mysterious ORCs. They rule out supernova remnants and galactic planetary nebulas because of their rarity. Several of the ORCs were spotted in one image, so if they turned out to be supernova remnants or galactic planetary nebulas, that would suggest that these objects are way more common than previously thought.

"[I]f the ORCs are [supernova remnants (SNRs)], which they strongly resemble, then this implies a population of SNRs in the Galaxy some 50 times larger than the currently accepted figure, or else a new class of SNR which has not previously been reported," they write.

Instead, the team suspects that ORCs may be a type of circular spherical wave which appeared in the aftermath of an extra-galactic transient event, like a powerful neutron star merger. They could also be a combination of different phenomena.

Alternatively, we could just be looking at a known object from a different perspective. "It is also possible that the ORCs represent a new category of a known phenomenon, such as the jets of a radio galaxy or blazar when seen end-on, down the barrel of the jet," they write.

One thing is clear: we need a lot more observations to unravel what exactly these objects might be.

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Astronomers Spot Strange Space Object, Have No Idea What It Is - Popular Mechanics

Astronomers think they can find the Sun’s lost siblings – Astronomy Magazine

Somewhere in the galaxy, we have a long-lost family. At this very minute, there are hundreds to thousands of stars that began to form and shine in the same dust cloud as our Sun, whose current locations are unknown in the sea of other stars. But what if it were possible to test stars to find our stellar siblings, like a DNA test can reveal unknown family members for humans on Earth? Astronomers think its doable and, whats more, we may have already done it.Although the Sun was born billions of years ago, we know roughly how the process happened by studying stellar nurseries we see today, called nebulae. Nebula means cloud in Latin, and each consists of interstellar gas, primarily hydrogen and helium with trace amounts of other elements. Many nebulae are inert, with no star formation happening in them, their presence betrayed only by the dark regions they form as they block light from more distant stars. In fact, if these dark nebulae did not exist, the Milky Way in our night sky would be much brighter. On the other hand, nebulae that are home to star formation are positively glowing, and several are so bright you can spot them with the naked eye.

Millions of years before the Sun formed, something disturbed the dark nebula containing the gas that would become our solar system. Astronomers believe they know what caused it: a massive explosion from a dying star, called a supernova.

A blast wave from a supernova can trigger star formation in the shock front [the leading edge of the explosion] if the material is dense enough, explains Anna Rosen, an astrophysicist at the Harvard-Smithsonian Center for Astrophysics. The key to this origin is locked in a surprising location: meteorites.

Meteoroids as meteorites are known when still in space are small chunks primarily made of iron, nickel, and trace amounts of other materials. The composition of most has not changed since the solar system formed; whats more, because they are the only part of outer space that can be physically carried into a laboratory on Earth, they are well studied. In examining them, scientists have discovered elements in amounts only possible if a supernova occurred just tens of thousands of years before the meteorites formed.

We see further evidence all around us. The elements in our world (except hydrogen and helium) formed in stars that died before our Sun was born, from the carbon in your cells to the oxygen in your lungs to the iron in your veins. These elements were then part of the material in our parent nebula that ended up forming Earth. As Carl Sagan said, We are made of starstuff.

After the supernovas shock wave passed through the cloud that would become the solar system, the dust and gas began to collapse in on itself due to gravity. More and more material fell onto it, forming a dense core, known as a protostar, that would become the Sun, and a protoplanetary disk of gas that would eventually become the rest of the solar system.

The Sun was not yet shining at this point. A protostar is not yet fusing hydrogen, so no ancient aliens would see our developing Sun, at least in wavelengths of visible light. There would be a lot of heat from all the collapsing gas, however, so the system would emit infrared radiation. Altogether, the Sun probably spent half a million years as a protostar, although accreting gas in the earlier stages could have taken many times longer.

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Astronomers think they can find the Sun's lost siblings - Astronomy Magazine

Astronomers Find Stellar Stream of Extragalactic Origin in the Vicinity of the Sun | Astronomy – Sci-News.com

A team of astronomers from Israel and the United States has discovered a vast stream of 250 stars of extragalactic origin in the vicinity of our Solar System.

Stellar streams arcing high over the Milky Way Galaxy are remnants of accreted dwarf galaxies and star clusters. Image credit: NASA / JPL-Caltech / R. Hurt, SSC & Caltech.

Galaxies form by swallowing other galaxies, said lead author Dr. Lina Necib, a postdoctoral researcher in the Walter Burke Institute for Theoretical Physics at Caltech.

Weve assumed that the Milky Way had a quiet merger history, and for a while it was concerning how quiet it was because our simulations show a lot of mergers.

Now, with access to a lot of smaller structures, we understand it wasnt as quiet as it seemed.

Its very powerful to have all these tools, data and simulations. All of them have to be used at once to disentangle this problem.

Were at the beginning stages of being able to really understand the formation of the Milky Way.

Dr. Necib and colleagues developed a method of tracking the movements of stars in virtual galaxies and labeling the stars as either born in the host galaxy or accreted as the products of galaxy mergers.

The two types of stars have different signatures, though the differences are often subtle.

These labels were used to train the deep learning model, which was then tested on simulations from the FIRE (Feedback In Realistic Environments) project.

After they built their catalogue of accreted stars, the astronomers applied it to the second data release from ESAs star-mapping satellite Gaia.

We asked the neural network, Based on what youve learned, can you label if the stars were accreted or not? Dr. Necib said.

The researchers first checked to see if it could identify known features of the Milky Way Galaxy.

These include the Gaia sausage, the remains of a dwarf galaxy that merged with the Milky Way about 6-10 billion years ago and that has a distinctive sausage-like orbital shape.

It has a very specific signature. If the neural network worked the way its supposed to, we should see this huge structure that we already know is there, Dr. Necib said.

The Gaia sausage was there, as was the stellar halo, and the Helmi stream, another known dwarf galaxy that merged with the Milky Way in the distant past and was discovered in 1999.

The model identified another structure in the analysis: a cluster of 250 stars, rotating with the Milky Ways disk, but also going toward the Galactic center.

Your first instinct is that you have a bug, Dr. Necib said.

And youre like, Oh no! So, I didnt tell any of my collaborators for three weeks. Then I started realizing its not a bug, its actually real and its new.

The authors argue that the newfound stellar stream, named Nyx, is a remnant of a disrupted dwarf galaxy that merged with the Milky Way billions years ago.

The Nyx stream provides the first indication that such an event occurred in the Milky Way, they said.

Such stellar streams are thought to be globular clusters or dwarf galaxies that have been stretched out along its orbit by tidal forces before being completely disrupted.

The scientists identified an additional stream, dubbed Nyx-2, with similar motion and stellar characteristics, but opposite velocity.

This suggests that Nyx-2 is related to Nyx and might actually be debris from a separate passage of the same satellite galaxy, they said.

The discovery is reported in the journal Nature Astronomy.

_____

L. Necib et al. Evidence for a vast prograde stellar stream in the solar vicinity. Nat Astron, published online July 6, 2020; doi: 10.1038/s41550-020-1131-2

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Astronomers Find Stellar Stream of Extragalactic Origin in the Vicinity of the Sun | Astronomy - Sci-News.com

Astronomers discover South Pole Wall, a gigantic structure stretching 1.4 billion light-years across – Livescience.com

Spectacular 3D maps of the universe have revealed one of the biggest cosmic structures ever found an almost-inconceivable wall stretching 1.4 billion light-years across that contains hundreds of thousands of galaxies.

The South Pole Wall, as it's been dubbed, has been hiding in plain sight, remaining undetected until now because large parts of it sit half a billion light-years away behind the bright Milky Way galaxy. The South Pole Wall rivals in size the Sloan Great Wall, the sixth largest cosmic structure discovered. (One light-year is roughly 6 trillion miles, or 9 trillion kilometers, so this "biggest cosmic structure" is mind-bendingly humongous.)

Astronomers have long noticed that galaxies are not scattered randomly throughout the universe but rather clump together in what's known as the cosmic web, enormous strands of hydrogen gas in which galaxies are strung like pearls on a necklace that surround gigantic and largely empty voids.

Related: Cosmic record holders: The largest objects in the universe

Mapping these intergalactic threads belongs to the field of cosmography, which is "the cartography of the cosmos," study researcher Daniel Pomarede, a cosmographer at Paris-Saclay University in France, told Live Science.

Previous cosmographic work has charted the extent of other galactic assemblies, such as the current structural record holder, the Hercules-Corona Borealis Great Wall, which spans 10 billion light-years, or more than a tenth the size of the visible universe.

In 2014, Pomarede and his colleagues unveiled the Laniakea supercluster, a galactic collection in which our own Milky Way resides. Lanaikea is 520 million light-years wide and contains roughly the mass of 100 million billion suns.

For their new map, the team used newly-created sky surveys to peer into a region called the Zone of Galactic Obscuration. This is an area in the southern part of the sky in which the bright light of the Milky Way blocks out much of what's behind and around it.

Cosmographers typically determine the distance to objects using redshift, the speed at which an object is receding from Earth due to the expansion of the universe, which depends on their distance, Pomarede said. The farther away an object is, the faster it will appear to be receding from Earth, an observation first made by astronomer Edwin Hubble in 1929 and which has held up ever since.

But he and his colleagues used a slightly different technique, looking at the peculiar velocity of galaxies. This measurement includes redshift but also takes into account the motion of galaxies around one another as they tug at each other gravitationally, Pomarede said.

The advantage of the method is that it can detect hidden mass that is gravitationally influencing how galaxies move and therefore uncover dark matter, that invisible stuff that emits no light but exerts a gravitational tug on anything near enough. (Dark matter also makes up the bulk of the matter in the universe.) By running algorithms looking at peculiar motion in galactic catalogs, the team was able to plot the three-dimensional distribution of matter in and around the Zone of Galactic Obscuration. Their findings are detailed today (July 9) in The Astrophysical Journal.

The resulting map shows a mind-boggling bubble of material more or less centered on the southernmost point of the sky, with a great sweeping wing extending north on one side in the direction of the constellation Cetus and another stubbier arm opposite it in the direction of the constellation Apus.

Related: The 12 strangest objects in the universe

Knowing how the universe looks on such large scales helps confirm our current cosmological models, Neta Bahcall, an astrophysicist at Princeton University in New Jersey who was not involved in the work, told Live Science. But determining where exactly these enormous, crisscrossing structures begin and end is tricky, she added.

"When you look at the network of filaments and voids, it becomes a semantic question of what's connected," she said.

In their paper, the team acknowledges that they may not have plotted yet the entirety of the vast South Pole Wall. "We will not be certain of its full extent, nor whether it is unusual, until we map the universe on a significantly grander scale," they wrote.

Originally published on Live Science.

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Astronomers discover South Pole Wall, a gigantic structure stretching 1.4 billion light-years across - Livescience.com

With backyard astronomy, the sky’s the distance – Vanguard – Psuvanguard.com

It is understandable to want to go outside now and it is a realistic desire to want to do things with peopleanything. COVID-19 has all but shut down venues of hobby, socializing and general activity that is not slowly creeping down a grocery aisle, face masked and shopping cart handles still wet from disinfectant.

Enjoying peoples company and engaging in a collective activity is not a far-off dream, however; backyard astronomy, the exploration of space from the comfort of your backyard, balcony or bedroom, offers a way to join in a community-based activity that does not require careful choreographing of ones social distance.

Backyard astronomy can be a low-barrier hobby, especially when starting out, stated Jim Todd of the Rose City Astronomers Club. The simple act of standing outside at night and looking up at the sky is the very best way to get started.

The number of accessible activities within the realm of what constitutes backyard astronomy might seem hard to narrow down, and Todd added the amount available to learn can often seem daunting.

In July alone, its possible to see a penumbral lunar eclipse (July 4), the brightest phase of recently discovered Comet NEOWISE (July 56), this years closest approach of Jupiter (July 14) and Saturn (July 20) and the Delta Aquariid meteor shower (July 2829).

Without a telescope, these events are still easily visible to the naked eye. 20 meteors are visible a minute during the Delta Aquariid meteor shower and the penumbral lunar eclipse, when the moon passes through Earths outer shadow is a multi-hour event. Meanwhile, a pair of binoculars can greatly enhance the view of the oppositions of Jupiter and Saturn.

For truly accessible viewing, radio receivers like the online setup at livemeteors.com can capture the sounds of meteors entering the atmosphere, providing an audio or haptic experience for those with difficulty seeing.

Meanwhile, those who desire an optical enhancement can consider the option of joining an astronomy club in their city. RCAs Todd pointed out many clubs offer telescopes for members to check out for a time. These arrangements provide club members the opportunity to take home a telescope to use for a variety of purposes, from astrophotography to basic viewing. And although COVID-19 has put these lending functions on hold, club functions have for the most part moved online for clubs throughout the country, including interest groups focused on optical viewing.

Why spy the sky?

It is generally accepted that social distancing can slow the spread of COVID-19, especially true social distancing involving staying home. Science agrees with the concept of staying home to save lives, therefore activities done entirely at home on your own are extremely successful at both keeping you busy and keeping you healthy.

The idea of a quarantine cosmic jaunt is thus an important consideration when you are tired of sitting at home.

Heres the thing: that sky youre looking at is almost certainly the same sky everyone else can see when they turn their eyes heavenward. Allowing for transient and localized events like bolides (fiery, extra bright meteors that explode) and short-lived phenomena like noctilucent clouds (electric-blue high atmospheric clouds), things in the night sky beyond the reach of our lower atmosphere do not actually change that quickly. In the case of the moon, for example, a quick glance at the moon two hours after a friend tells you to go check it out will only mean a roughly .2% change in phase. That might mean a lot if you are interested in checking out a crater on the edge of the earths shadow, but in the grand scheme of things, Lunas orb appears unchanged.

In the context of social distancing and public health, this kind of community activity is incredibly important.

There is also the proliferation of astronomy and space science online that can provide this same kind of connection with your neighbors, so even if the sky is cloudya fair bet in Portlandthe wonders of the sky in their current form are still largely accessible, barring some kind of worldwide outbreak of Oregon gloom.

This is where the mental health benefits of backyard astronomy make themselves known. You can easily immerse yourself in a generations-long fascination with the stars and planets uncountable without leaving your personally defined safety bubble. That longing for any kind of association with people can be met in large part by turning your eyes, ears or haptic device toward the sky.

Learning your lines

Rose City Astronomers Todd was open about the possibilities for learning beyond just the grasping of the mere existence of phenomena in the sky. He also tamped down any expectation of a difficult, perhaps stereotypically nerdy and difficult hobby. All of these tips could sound intimidating on your own. However, they are simple if you go to a star party or club event. You can talk to other beginners as well as experts and start to find your way toward what interests you, Todd stated.

To that end, Todd provided resources for the beginning stargazer. Websites like Stellarium, In The Sky and The Sky Live offer means of getting your bearings around the starry depths. Heavens Above, NASAs Solar Dynamics Observatory and SpaceWeather.com give the beginner and expert alike a chance to step beyond just distant stars and nearby planets in their celestial viewing. Astronomy Picture of the Day, updated daily without fail, provides a carefully curated gallery of space that touches on all aspects, from method to Pulitzer-worthy digital tableau.

A quick glance at Vanguards bookshelf also shows that old-fashioned paper and bindings provide guidepost and interpretation of the night sky. Books like the venerable Peterson First Guide to Astronomy and Petersons Field Guide to Stars and Planets, Chet Raymos 365 Starry Nights, Golden Guides Stars, Terence Dickinsons NightWatch and Alan Dyers The Backyard Astronomers Guide provide a starter library of classic texts.

Scientific exploration by curious and starry-eyed social distancers is thus worth all the stars in the sky.

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Astronomy Enthusiasts Look Forward to Spotting International Space Station Tonight – The New Leam

There is some exciting news for astronomy lovers throughout the country and especially for inhabitants of Rajkot, Ahmedabad and Delhi. This is because the International Space Station will be spotted in the night sky. This is not an altogether rare phenomenon but it will nevertheless excite astronomy lovers in these cities.

The space station will appear like a bright star when one looks at it through plain eyes as it is considered to be the third biggest object in the sky after the Sun and Moon. The space station completes one round around the earth in roughly 93 minutes and does 15.5 orbits every day.

The clarity of vision that is gained from these cities will be due to the fact that the space station will fly right over these cities at an angle of 90 degrees and give autonomy enthusiasts the perfect chance to look the satellite if the skies in the respective cities remain clear.

The space station will be visible after 8.30 pm. It will be seen after 8.30 pm in these cities. These four cities are likely to have the best sightings if the skies are clear.

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Astronomy Enthusiasts Look Forward to Spotting International Space Station Tonight - The New Leam

Astronomers Observe Most Distant Explosion in Universe That Took Place 10 Billion Years Ago – Gadgets 360

Astronomers have spotted one of the most powerful and oldest explosions that took place nearly 10 billion years ago. The explosion that has been named SGRB181123B occurred just 3.8 billion years after the Big Bang - the cosmological event that led to the formation of our universe. Astronomers claim that the discovery offered a "rare opportunity" to study the neutron star mergers from when the universe was a "teenager." It is also said to be the second most-distant, well-established short gamma ray burst (SGRB) ever detected and the most distant event "with an optical afterglow."

The research was published on Tuesday in the Astrophysical Journal Letters. Speaking more about SGRB181123B explosion that happened nearly 10 billion light-years away, a Northwestern University press release citing the senior author of the study, Wen-fai Fong indicated that its discovery was a combination of luck and quick action.

"We certainly did not expect to discover a distant SGRB, as they are extremely rare and very faint...We perform 'forensics' with telescopes to understand its local environment because what its home galaxy looks like can tell us a lot about the underlying physics of these systems," a Fong stated.

SRGBs are described as the most energetic and brightest forms of explosions in the universe that occur after the merger of two neutron stars. Typically, astronomers detect nearly eight SRGBs each year; however, they are hard to study as their afterglow only lasts for an hour or so.

"With SGRBs, you won't detect anything if you get to the sky too late. But every once in a while, if you react quickly enough, you will land on a really beautiful detection like this," Fong added.

The SGRB181123B explosion was first detected in 2018 by the NASA's Neil Gehrels Swift Observatory. Hours after its detection, the Northwestern team remotely accessed the International Gemini Observatory, using the Gemini-North telescope, located atop Mauna Kea in Hawaii. Following this, researchers measured SGRB181123B's optical afterglow using an 8.1-meter telescope.

After this point, more follow-up observations from Chile and Arizona indicated the origin of the explosion.

"Finding an SGRB at this point in the universe's history suggests that, at a time when the universe was forming lots of stars, the neutron star pair may have merged fairly rapidly," Wong said.

Why do Indians love Xiaomi TVs so much? We discussed this on Orbital, our weekly technology podcast, which you can subscribe to via Apple Podcasts, Google Podcasts, or RSS, download the episode, or just hit the play button below.

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Astronomers Observe Most Distant Explosion in Universe That Took Place 10 Billion Years Ago - Gadgets 360