The Condor Array Telescope: Unlocking the Mysteries of the Very-Low-Brightness Universe

Monday - March 18 2024, 02:25 UTC - 8 months ago

The Condor Array Telescope, a collaboration between Stony Brook University and the American Museum of Natural History, has recently published its first scientific findings. By using computers to combine light from smaller telescopes, Condor is able to detect and study extremely faint astronomical features. Its achievements include clarifying the nature of stellar streams and discovering new gas shells, showcasing its ability to capture faint features.

A new telescope called the “Condor Array Telescope” may open up a new world of the very-low-brightness Universe for astrophysicists. Four new papers, published back to back in the Monthly Notices of the Royal Astronomical Society (MNRAS) this month, present the first scientific findings based on observations acquired by Condor. The project is a collaborative led by scientists in the Department of Physics and Astronomy at Stony Brook University and the American Museum of Natural History (AMNH) .

According to lead researchers Kenneth M. Lanzetta, PhD, a Professor in the Department of Physics and Astronomy and Stefan Gromoll of Stony Brook, and Michael M. Shara, PhD, Curator in the Department of Astrophysics at the AMNH, Condor is now in full operation. The new “array telescope” uses computers to combine light from several smaller telescopes into the equivalent of one larger telescope and is able to detect and study astronomical features that are too faint to be seen with conventional telescopes .

In the first paper,[1] Lanzetta and colleagues used Condor to study extremely faint “stellar streams” surrounding the nearby galaxy NGC 5907, a well-known spiral galaxy located some 50 million light years from Earth. Such streams are produced when dwarf companion galaxies are disrupted by the tidal gravitational force of the primary galaxy. A previous image obtained by a different telescope in 2010 appeared to show a remarkable stellar stream forming two complete loops of a helix surrounding the galaxy .

But another image obtained by the “Dragonfly Telephoto Array” in 2019 showed no trace of this helix. The Condor team decided to test the new array telescope and to weigh in on the discrepancy. They obtained a deep image of NGC 5907 in 2022. Like the Dragonfly image, the Condor image showed no trace of the helix, leading the team to conclude that the helix of the 2010 image was likely an artifact related to the image processing .

The Condor image also revealed faint features that were not picked up by the previous images. In the second paper,[2] Shara and colleagues used Condor to reassess an image of the dwarf nova Z Camelopardalis or “Z Cam” obtained by the Kitt Peak National Observatory 4-meter telescope back in January 2007. The image showed a partial shell of gas surrounding Z Cam, which Shara speculated was emitted by a “new star” recorded by Chinese Imperial astrologers in the year 77 BCE .

To test this speculation, the Condor team obtained a new image of Z Cam in November 2021. Then by comparing the positions of the shell in the earlier and later images, they measured the expansion rate of the shell, finding a rate that is indeed consistent with an explosion more than 2000 years ago. But to their astonishment, the team found that the new Condor image revealed the complete shell of gas surrounding Z Cam, underscoring the telescope's ability to capture faint astronomical features .