Gemini Observatory, using the Near-Infrared Integral Field Spectrograph on the Gemini North telescope in Hawai‘i, has confirmed the spiral nature of what is now the most distant known spiral galaxy. The galaxy's light, revealing how the galaxy looked some 11 billion years ago, is gravitationally lensed by a massive foreground cluster of galaxies to help reveal the distant pinwheel nature of the galaxy.
The following is a press release from Swinburne University of Technology in Australia.
The most ancient spiral galaxy discovered to date is revealing its secrets to a team of astronomers at Swinburne University of Technology and the Australian National University (ANU), both part of the Australian Research Council Centre of Excellence in All Sky Astrophysics in 3D (ASTRO 3D).
The galaxy, known as A1689B11, existed 11 billion years in the past, just 2.6 billion years after the Big Bang, when the Universe was only one fifth of its present age. It is thus the most ancient spiral galaxy discovered so far.
The researchers used a powerful technique that combines gravitational lensing with the cutting-edge instrument, the Near-infrared Integral Field Spectrograph (NIFS) on the Gemini North telescope in Hawai‘i, to verify the vintage and spiral nature of this galaxy. NIFS is Australia’s first Gemini instrument that was designed and built by the late Peter McGregor at the ANU.
Gravitational lenses are Nature’s largest telescopes, created by massive clusters composed of thousands of galaxies and dark matter. The cluster bends and magnifies the light of galaxies behind it in a manner similar to an ordinary lens, but on a much larger scale.
“This technique allows us to study ancient galaxies in high resolution with unprecedented detail,” says Swinburne astronomer Dr Tiantian Yuan, who led the research team.
“We are able to look 11 billion years back in time and directly witness the formation of the first, primitive spiral arms of a galaxy.”
Co-author, Princeton University’s Dr Renyue Cen, says: “Studying ancient spirals like A1689B11 is a key to unlocking the mystery of how and when the Hubble sequence emerges.”
“Spiral galaxies are exceptionally rare in the early Universe, and this discovery opens the door to investigating how galaxies transition from highly chaotic, turbulent discs to tranquil, thin discs like those of our own Milky Way galaxy.”
Dr Yuan says the study shows some surprising features of A1689B11.
“This galaxy is forming stars 20 times faster than galaxies today – as fast as other young galaxies of similar masses in the early Universe. However, unlike other galaxies of the same epoch, A1689B11 has a very cool and thin disc, rotating calmly with surprisingly little turbulence. This type of spiral galaxy has never been seen before at this early epoch of the Universe!”
This research is an international collaboration including astrophysicists from the University of Lyon in France, Princeton University in the USA and Hebrew University in Israel. It has been accepted for publication in The Astrophysical Journal. A preprint version is available here.
Science Contacts:
Tiantian Yuan
Swinburne University of Technology
Email: tiantianyuan@swin.edu.au
Desk: +613 9214 5948
Cell: +61 404 029 550
Media Contacts:
Lea Kivivali
Swinburne University of Technology
Email: lkivivali@swin.edu.au
Desk: +613 9214 5428
Cell: +61 410 569 311
Peter Michaud
Public Information and Outreach Manager
Gemini Observatory
Hilo, Hawai‘i
Email: pmichaud@gemini.edu
Desk: 808 974-2510
Cell: 808 936-6643
Source: Gemini Observatory
