AstronomyHow a discovery at a Hawaii volcano sparked a project with a history unlike anything else on campus
The unassuming observatory dome on the roof of the Physics and Biology Research Building, while unused today, has a storied past. Photo by Jackie Ricciardi
Every day, hundreds of BU students walk down Cummington Mall, unaware that they are passing by a fascinating and unique campus relic, with a story full of drama, mystery, near-disaster, and earth-shattering scientific intrigue.
The unassuming observatory dome on the roof of the Physics and Biology Research Building (PRB) has a storied past: it was built to house a telescope that was eventually used at the South Pole.
The story of this observatory began in 1990 when astronomers at Mauna Kea, a mostly underwater volcano on the island of Hawaii, detected carbon in interstellar clouds that was 10 times brighter than anyone had expected. Interstellar clouds are accumulations of gas, dust, and plasma between star systems in a galaxy. Astronomers can determine the chemical compositions of these clouds by studying the radiation they emanate. The unexpected abundance of carbon detected on Mauna Kea was excitingit could point to something new in the field of astronomy.
The notion was that there may be a lot of atomic carbon that weve never properly mapped, says Thomas Bania, a College of Arts & Sciences professor of astronomy. Carbon is a very important atomic element, and if theres a whole lot of carbon in atomic form that we dont know about, it completely changes the way we study the chemistry of the interstellar medium and the chemistry of molecular clouds, things like that. Detecting that much more carbon would radically change our understanding of the composition of significant portions of the Milky Way Galaxy, transforming our understanding of galactic evolution, the formation of stars and planets, and perhaps even the origin of life in the universe.
Eager to follow this lead, Anthony Stark, an astrophysicist at the Harvard Smithsonian Center for Astrophysics, teamed up with Bania and a team of astronomers from BU and Harvard to create the Antarctic Submillimeter Telescope and Remote Observatory (AST/RO) project. Their group included BU astronomy doctoral students Maohai Huang (GRS00), Alberto Bolatto (GRS01), James Ingalls (GRS98), and undergraduate Edgar Castro (ENG95). Together, they set out to design and build a telescope from scratchone that they would eventually send all the way down to the South Pole for carbon observations.
Observational astronomers run into all sorts of issues when trying to operate a telescope in warmer environments: high wind speeds can shake the instruments, rapid temperature fluctuations cause metal and glass in the telescope to expand and contract, wet weather can damage the sensitive instrumentation, and nosy animals or errant birds can interfere with the telescope.
But these arent issues at the South Pole. It may not be a livable environment, but for over a century, astronomers have been conducting science in this inhospitable place, because with all the inconveniences of moderate climates, scientists have decided the benefits of what they might learn there make getting a bit cold worthwhile.
From 1990 to 1992, the AST/RO telescope was built from scratch at Bell Laboratories in New Jersey and BUs Scientific Instrument Facility in the PRB basement. Its design is called offset Gregorian: once light enters the telescope, it bounces off four mirrors that direct it into a room below, called a Coud room, where it is focused into an image.
As the telescope was being built, a team of BU Facilities Management & Planning workers constructed the test dome on the PRB roof. This was an ideal place to test the telescope since the rooftop had a clear view of the southern horizon (the Life Science & Engineering Building wasnt there yet). One challenge, though, would be getting the telescope up there. The elevator goes only as high as the fifth floorfrom there you have to climb another flight of stairs and then a ladder to get to the porthole that opens onto the roof. The AST/RO researchers made this climb every time they had to get to the observatory. That ladder is still the only way to get to the roof.
There was no way they could bring the telescope in pieces, one by one, up the ladder and through the two-foot-by-two-foot porthole. So the team installed a small crane inside the dome and used it to lift several of the telescope pieces from the fifth floor, through a series of hatchwaysand through a biology labto the observatory. The biggest telescope pieces had to be hoisted onto the roof from a crane outside the building.
Once everything was assembled on the roof, the team spent 18 months testing the instrumentation. Huang remembers spending many long nights at the test site, even taking naps in the control room below the telescope. But every so often, he would wander up to the rooftop dome and enjoy a few quiet moments in the Boston morning. There is nobody there, of course, he says, as the sun is just beginning to crest over the city skyline in the east, and you can see very faryou can see the Charles River, and everything.
In 1995, the AST/RO telescope was finally ready for the South Pole. The team packed it up in a green-painted wooden crate (nicknamed the Green Monster). Its journey to the South Pole took three weeks and multiple modes of transportation: Boston to Los Angeles via truck, Los Angeles to McMurdo Station in Antarctica by ship, then McMurdo to the Amundsen-Scott South Pole Station aboard a C130 military plane.
But it did not go gentle: on the first leg of the trip, the truck carrying it crashed on a highway near Little Rock, Ark. Bania recalls going down to assess the damage with James Jackson, a CAS adjunct professor of astronomy. We had the telescope, all of its computers, all of its electronics, all of the spares, all of the tools that it was going to take to put it back together, all of the documentation for an entire state-of-the-art high-frequency radio observatory in one truck, says Bania. He and Jackson had to decide if it was worth the risk to send the telescope down to the South Pole, or if they should just bring it back to Boston and take stock of the damage there, losing a year in the process.
They decided to send it down to Antarctica. Fortunately, their gamble paid offthe telescope arrived in working condition.
The AST/RO telescope operated at the South Pole from 1995 to 2001. Bania and his students went down every year during the Antarctic summer (winter in the Northern Hemisphere) to perform maintenance and keep it operational.
In the end, though, the project was deemed a flop. After 10 years of work, it turned out that, no, carbon was brighter for a different reasonand so there wasnt this vast reservoir of atomic carbon, Bania says. And proving a negative never leads to a sexy press release.
With that, AST/RO was unceremoniously boxed back up and left in a graveyard of other abandoned scientific instruments at the South Pole. Its now probably buried under ice.
For those who spent hours, days, weeks, and years of their lives on the project, however, it was hardly a flop; all four BU grad students who worked on it got their doctorates and are still doing astronomy research. Huang, for example, is a research professor at the National Astronomical Observatory of China, where he works on the science operation and data processing system for astronomical systems, including the Herschel Space Observatory. What I learned from AST/RO really directly goes into what Im working on now, Huang says. Controlling AST/RO was as difficult as controlling a telescope in space, he says: both are hard to access, so youd better make sure things work the first time. If something breaks, its going to take a very long time to fix.
And, almost 30 years later, the AST/RO test dome remains atop the southwest corner of PRB, a monument to the teams decade of work.
For those researchers like Bania, it stirs up mixed memories. On bad days, I think I wasted 10 years of my life, he says. On good days, I think, well, you know, I had the opportunity to build an observatory from the ground up and operate it. Not many people can say that.
The rest is here:
- Rotational spectra of isotopic species of methyl cyanide, CH_3CN, in their ground vibrational states up to terahertz frequencies [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Cosmological parameter extraction and biases from type Ia supernova magnitude evolution [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Continuous monitoring of pulse period variations in Hercules X-1 using Swift/BAT [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Constraining the ortho-to-para ratio of H{_2} with anomalous H{_2}CO absorption [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- A photometric and spectroscopic study of the new dwarf spheroidal galaxy in Hercules - Metallicity, velocities, and a clean list of RGB members [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Luminosities and mass-loss rates of SMC and LMC AGB stars and red supergiants [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Electron beam – plasma system with the return current and directivity of its X-ray emission [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- The propagation of the shock wave from a strong explosion in a plane-parallel stratified medium: the Kompaneets approximation [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Analysis of hydrogen-rich magnetic white dwarfs detected in the Sloan Digital Sky Survey [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Letter: Centaurus A as TeV \gamma-ray and possible UHE cosmic-ray source [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Young pre-low-mass X-ray binaries in the propeller phase - Nature of the 6.7-h periodic X-ray source 1E 161348-5055 in RCW 103 [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Radiative rates and electron impact excitation rates for transitions in Cr VIII [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Solar granulation from photosphere to low chromosphere observed in Ba II 4554 Å line [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Does the HD 209458 planetary system pose a challenge to the stellar atmosphere models? [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Effect of asymmetry of the radio source distribution on the apparent proper motion kinematic analysis [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Destriping CMB temperature and polarization maps [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Search for cold debris disks around M-dwarfs. II [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Precise data on Leonid fireballs from all-sky photographic records [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- An X-ray view of 82 LINERs with Chandra and XMM-Newton data [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Radio observations of ZwCl 2341.1+0000: a double radio relic cluster [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Candidate free-floating super-Jupiters in the young \sigma Orionis open cluster [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- The metallicity gradient as a tracer of history and structure: the Magellanic Clouds and M33 galaxies [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- XMMSL1 J060636.2-694933: an XMM-Newton slew discovery and Swift/Magellan follow up of a new classical nova in the LMC [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- The inner rim structures of protoplanetary discs [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- The solar Ba{\sf II} 4554 Å line as a Doppler diagnostic: NLTE analysis in 3D hydrodynamical model [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Magnetic evolution of superactive regions - Complexity and potentially unstable magnetic discontinuities [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Low-mass protostars and dense cores in different evolutionary stages in IRAS 00213+6530 [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- PMAS optical integral field spectroscopy of luminous infrared galaxies - I. The atlas [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- First AGILE catalog of high-confidence gamma-ray sources [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Radiative hydrodynamics simulations of red supergiant stars - I. interpretation of interferometric observations [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Extrasolar planets and brown dwarfs around A–F type stars - VII. \theta Cygni radial velocity variations: planets or stellar phenomenon? [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Cosmic rays and the magnetic field in the nearby starburst galaxy NGC 253 - II. The magnetic field structure [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Physical structure and water line spectrum predictions of the intermediate mass protostar OMC2-FIR4 [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- The bright galaxy population of five medium redshift clusters - II. Quantitative galaxy morphology [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Dust in brown dwarfs and extra-solar planets - II. Cloud formation for cosmologically evolving abundances [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- The quiet Sun magnetic field observed with ZIMPOL on THEMIS - I. The probability density function [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Complexity in the sunspot cycle [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Properties and nature of Be stars - 26. Long-term and orbital changes of \zeta Tauri [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- The massive Wolf-Rayet binary LSS 1964 (=WR 29) - II. The V light curve [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Supernova progenitor stars in the initial range of 23 to 33 solar masses and their relation with the SNR Cassiopeia A [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- The Hertzsprung-Russell Diagram of Star Clusters [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Table of the 10 Brightest stars within 10 Parsecs of the Sun [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- The Hertzsprung-Russell Diagram of the Nearest Stars [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Magnitude and Color in Astronomy [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Stellar Types [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Brown Dwarfs [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Spotting the Minimum [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- The Structure and Evolution of Brown Dwarfs [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- No Bang from the Big Bang Machine [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- The Sizes of the Stars and the Planets [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- An Implausible Light Thrust [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- the Masses of Degenerate Objects [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Degeneracy Pressure [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Introduction to Degenerate Objects [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- The Radii of Degenerate Objects [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- The Inevitability of Black Holes [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Scientific Pig-Out [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- The Neutrino Cooling of Degenerate Dwarfs [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- The Neutrino Cooling of Neutron Stars [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Overview of Supernovae [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Energetics of Thermonuclear Supernovae [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Thermonuclear Supernovae [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Nuclear Reactions in Thermonuclear Supernovae [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Core-Collapse Supernovae [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Neutrinos and SN 1987A [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Revealing the sub-AU asymmetries of the inner dust rim in the disk around the Herbig Ae star R Coronae Austrinae [Last Updated On: December 13th, 2009] [Originally Added On: December 13th, 2009]
- Probing the dust properties of galaxies up to submillimetre wavelengths - I. The spectral energy distribution of dwarf galaxies using LABOCA [Last Updated On: December 13th, 2009] [Originally Added On: December 13th, 2009]
- On the physical origin of the second solar spectrum of the Sc II line at 4247 Å [Last Updated On: December 13th, 2009] [Originally Added On: December 13th, 2009]
- On detecting the large separation in the autocorrelation of stellar oscillation times series [Last Updated On: December 13th, 2009] [Originally Added On: December 13th, 2009]
- Imaging the spotty surface of Betelgeuse in the H band [Last Updated On: December 13th, 2009] [Originally Added On: December 13th, 2009]
- Chandra observation of Cepheus A: the diffuse emission of HH 168 resolved [Last Updated On: December 13th, 2009] [Originally Added On: December 13th, 2009]
- A planetary eclipse map of CoRoT-2a - Comprehensive lightcurve modeling combining rotational-modulation and transits [Last Updated On: December 13th, 2009] [Originally Added On: December 13th, 2009]
- The chemical composition of carbon stars. The R-type stars [Last Updated On: December 13th, 2009] [Originally Added On: December 13th, 2009]
- Flow instabilities of magnetic flux tubes - IV. Flux storage in the solar overshoot region [Last Updated On: December 13th, 2009] [Originally Added On: December 13th, 2009]
- Fragmentation of a dynamically condensing radiative layer [Last Updated On: December 13th, 2009] [Originally Added On: December 13th, 2009]
- Temporal variations of the CaXIX spectra in solar flares [Last Updated On: December 13th, 2009] [Originally Added On: December 13th, 2009]
- Deuterium chemistry in the Orion Bar PDR - “Warm” chemistry starring CH_{2}D^+ [Last Updated On: December 13th, 2009] [Originally Added On: December 13th, 2009]
- Metal abundances in the cool cores of galaxy clusters [Last Updated On: December 13th, 2009] [Originally Added On: December 13th, 2009]
- The nature of the X-ray binary IGR J19294+1816 from INTEGRAL, RXTE, and Swift observations [Last Updated On: December 13th, 2009] [Originally Added On: December 13th, 2009]
- Relating basic properties of bright early-type dwarf galaxies to their location in Abell 901/902 [Last Updated On: December 13th, 2009] [Originally Added On: December 13th, 2009]