NRAO March Tip Sheet

Science, Engineering, and Technology Milestones

Article ID: 615622

Released: 26-Mar-2014 10:00 AM EDT

Source Newsroom: National Radio Astronomy Observatory

  • Credit: L. Perez (NRAO/AUI/NSF); B. Saxton (NRAO/AUI/NSF); T. Muto (Tokyo Institute of Technology); NAOJ/Subaru

    This composite image of the protoplanetary disk SAO 206462 shows the distribution of dust around the young star. The red area indicates where ALMA observed the lopsided dust concentration. This vortex feature may be a crucial step in the formation of planets. The diffuse blue region is the emission from the dust surrounding the star. The apparent spiral features as seen in the infrared (white/light blue) may trace the presence of an unseen object, possibly a planet, perturbing the system. Further observations with ALMA and the VLA are necessary to confirm the spiral nature of this feature.

  • Credit: L. Perez (NRAO/AUI/NSF); B. Saxton (NRAO/AUI/NSF); K. Follette (Univ. Arizona); NAOJ/Subaru

    This composite image of the protoplanetary disk SR 21 shows the distribution of dust around the young star. The lower (pink/red) section indicates where ALMA observed the lopsided dust concentrations around this star. The blue and green regions are extended areas of dust as seen in the infrared.

1. Astronomers Make Best Measurement Yet of Distance to Galactic Center: An ongoing project using NRAO's Very Long Baseline Array (VLBA), the European VLBI Network, and the Japanese VERA project has produced the most accurate measurement yet of the distance from the Earth to the center of our Milky Way Galaxy. The new measurement -- 27,190 light-years -- is accurate, astronomers said, to better than 2 percent.

"That is certainly more accurate than most road-sign mileages," said Mark Reid, of the Harvard-Smithsonian Center for Astrophysics. Improving this measurement, he added, is important because it affects scientists' determinations of distances, masses, and brightnesses of nearly all objects in the Galaxy.

This distance measurement came as the project published more than 100 direct distance measurements to star-forming regions in the Galaxy. The long-term effort is designed to make a detailed map of the structure of our Galaxy, including the locations of its spiral arms.

Mapping our own Galaxy is difficult because we are inside it. Mapping the Milky Way requires that astronomers measure the distances to objects within it, and distance measurement has long been a difficult astronomical problem. Using the super-sharp capabilities of the VLBA and other systems, astronomers can measure the subtle shift in an object's apparent position in the sky when viewed from opposite ends of the Earth's orbit around the sun. This technique, called parallax, produces accurate distance measurements using simple trigonometry.

Radio telescopes allow the scientists to use this technique to determine distances to distant star-forming regions, even though those regions are obscured from optical telescopes by gas and dust. The radio technique, the scientists said, produces measurements more accurate than those anticipated in 2020 from the recently launched European satellite Gaia.

However, Gaia will target upwards of one billion stars that can be seen away from the plane of the Milky Way, making the optical and radio projects quite complementary.

The new distance measurements, and more to come from this project, will give astronomers much better figures for the basic parameters of the Milky Way. The ultimate objective is to make the most-detailed map yet of our home Galaxy and, for the first time, learn what it really looks like.

2. Astronomers Bet on VEGAS to Study the Cosmos: Astronomers bet that the Robert C. Byrd Green Bank Telescope’s (GBT) new spectrometer – known as VEGAS – will be an easy win for the telescope. This upgrade to the GBT’s spectroscopic capabilities will help astronomers understand the context of star formation, the evolution of the Universe across cosmic time, and the origin of molecules that are essential for life.

Spectrometers are tools for teasing out and studying the specific wavelengths of light that are emitted naturally by objects in the cosmos. Like a prism that separates white visible light into its constituent colors, a spectrometer takes a sliver of the electromagnetic spectrum (in this case, radio light) and spreads it out. From this, astronomers detect spikes and dips in the spectrum, revealing the presence of specific atoms, molecules, and physical processes.

VEGAS is short for the VErsatile GBT Astronomical Spectrometer. It will replace all of the GBT’s current spectral-line instruments while also supporting the GBT’s new multi-pixel radio “camera” development program. VEGAS was developed by the NRAO in collaboration with the Center for Astronomy Signal Processing and Electronics Research (CASPER) at the University of California, Berkeley.

In its high-bandwidth mode, VEGAS will function like eight independent spectrometers, capable of processing radio light over a 10 GHz bandwidth. It also can process up to seven separate data feeds, each equivalent to a pixel on a digital camera. Initial observing with VEGAS began March 10, 2014.

3. Protoplanetary Disks ‘Bulge’ in Complex and Asymmetrical Ways: Astronomers using the Atacama Large Millimeter/submillimeter Array (ALMA) have studied two massive protoplanetary disks and discovered large-scale asymmetries in the way their dust is distributed. By comparing these results with other early ALMA observations, the researchers speculate that asymmetrical disks may be the norm and an essential step along the path to planet formation.

In these protoplanetary systems, dubbed SR 21 and SAO 206462, ALMA revealed dust-depleted disk cavities near the stars and gaseous disks extending farther into space. It was in these extended gaseous regions that the asymmetries in the dust were discovered.

“These observations revealed large-scale asymmetries in the outer portions of the disks, each containing as much material as two Jupiter-sized planets,” said astronomer Laura Perez with the National Radio Astronomy Observatory (NRAO) in Socorro, N.M. “The best fit to explain these observations is a vortex structure in the outer disk.”

Similar in some respects to other asymmetrical bulges known as “dust traps” seen in earlier ALMA observations, these vortices could help the dust and gas around stars to clump together more readily. Models predict that once dust grains achieve a certain size, they either would drift inward toward the star or collide with other similar-size grains. By concentrating dust and gas, these asymmetrical regions may provide a safe haven where grain growth can continue.

The vortices revealed in the new ALMA observations occupy a much wider swath of the disk than seen in previous observations, however. This may indicate that they formed under different conditions, possibly as the result of turbulence in the disk.

Both SR 21 and SAO 206462 are in the process of transforming from optically thick disks brimming with dust and gas to optically thin debris disks, potentially harboring fully formed planets. Earlier observations with other telescopes failed to detect these large asymmetrical regions. ALMA’s enhanced resolution and sensitivity, however, could discern these features.

Perez and her colleagues speculate the process (or processes) that create these asymmetries may be taking place in most transitional disks.

ALMA also detected residual structures that don’t quite fit into the vortex model. It’s possible these represent spiral structures in the disks, but future observations with ALMA and the Karl G. Jansky Very Large Array (VLA) are necessary to confirm this.

The results are published in Astrophysical Journal Letters. []

- - - - - - - - - -The National Radio Astronomy Observatory is a facility of the National Science Foundation, operated under cooperative agreement by Associated Universities, Inc.


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