News
Primordial Galaxy Discovered, First of Its Kind
MEDIA CONTACT:
Mari-Ela Chock, Communications Officer
W. M. Keck Observatory
(808) 554-0567
SCIENCE CONTACT:
Andy Fell, Associate Director, Research Communications
University of California, Davis
(530) 752-4533
Maunakea, Hawaii– Seven years of meticulous observing have resulted in a cosmic discovery that comes from an era dating back 13.1 billion years, giving scientists a detailed glimpse of what may have happened just after the Big Bang.
Using the world-class W. M. Keck Observatory on Maunakea, Hawaii, an international team of astronomers from the United States, Australia, and Europe has confirmed the existence of one of the most distant galaxies in the universe.
To characterize the faint galaxy, the discovery team, led by Austin Hoag, a University of California, Davis physics graduate student, used MOSFIRE, the most in-demand instrument on the 10-meter Keck I telescope.
What makes this galaxy extraordinary is that it is ordinary. It is thought to be a common galaxy at that distance and age of the universe. However, such galaxies would normally be too faint to detect. The astronomers used a method called gravitational lensing to magnify the galaxy so they could study it.
“Most objects that we’ve seen at that distance are extremely bright, and probably rare compared to other galaxies,” said Hoag. “We think this galaxy is much more representative of other galaxies of its time.”
The results publish today in Nature Astronomy, with Hoag as the lead author on the paper.
“I’m like a proud academic mother,” said Marusa Bradac, associate physics professor at UC Davis. “It is a wonderful opportunity for graduate students to use the world’s best facilities to discover first galaxies and get their research published in Nature Astronomy.”
Named MACS1423-z7p64, the galaxy is at a redshift of 7.6, meaning its light came from when the universe was approximately 700 million years old.
“This is an awesome discovery in that it is the faintest galaxy at that redshift ever detected. It is very challenging to find an object at the very edges of the universe. In order to detect this galaxy, its light had to be lensed twice – once by a massive galaxy cluster, and a second time by the Keck Observatory telescope,” said Keck Observatory instrument program manager Marc Kassis who, along with fellow support astronomers Luca Rizzi and Carlos Alvarez, helped support Hoag and his team.
To find such faint, distant objects, the discovery team took advantage of a method called gravitational lensing. As light of the distant object passes by a massive object such as a galaxy cluster in the foreground, it gets bent by gravity, just as light gets bent passing through a lens. When the foreground object is massive enough, it will magnify the object behind it.
MACS1423-z7p64 just happened to fall into the “sweet spot” behind a giant galaxy cluster that magnified its brightness tenfold and made it first visible to the team using the Hubble Space Telescope. They were then able to confirm its distance by analyzing its spectrum using Keck Observatory’s MOSFIRE.
Even though MACS1423-z7p64 is strongly magnified, the discovery has been extremely challenging and it required combining the initial data taken by UC Davis researchers in 2015 with those from a second night of Keck observations from Australian colleagues at the University of Melbourne in 2016.
“This detection of Lyman-α emission from the galaxy thus highlights the strength of collaborative research projects,” said Michele Trenti from the University of Melbourne, principal investigator of the Australian observations.
“This is yet another discovery that puts UC Davis, UCLA, and University of Melbourne on the map as among the top astronomy centers in their nations, and the reason for that is due to our access to the Keck telescopes,” said Bradac. “For this kind of research, every meter of telescope aperture counts, and without the low humidity on Maunakea, we would not have been able to discover this.”
What’s Next
The discovery team plans to continue surveying candidate galaxies with the Hubble and Keck telescopes. Hoag says the upcoming launch of the James Webb Space Telescope (JWST), set for 2018, opens up new possibilities. The team is currently planning observations for the Webb telescope, which is bigger than Hubble and will allow astronomers to look at even more distant parts of the universe. As such, the very distant galaxies discovered by Keck Observatory in collaboration with the Hubble Space Telescope are precious candidates for further investigation by JWST.
“We will truly witness the birth of the first galaxies, which will allow us to answer the longstanding question of, ‘Where did we come from?’” Bradac said.
Ultradistant galaxies are of interest to scientists because they date back to a period known as the “Epoch of Reionization” – about a billion years after the Big Bang when the earliest stars and galaxies began to emit visible light into the universe for the very first time. Having the ability to study this light could give researchers the data they need to piece together the first chapters of our cosmic history and trace the origin of celestial objects we see today, including stars like our own Sun.
About MOSFIRE
W. M. Keck Observatory’s instrument, the Multi-Object Spectrograph for Infrared Exploration (MOSFIRE), gathers spectra from objects spanning a variety of distances, environments and physical conditions. What makes this large, vacuum-cryogenic instrument unique is its ability to select up to 46 individual objects in the field of view and then record the infrared spectrum of all 46 objects simultaneously. When a new field is selected, a robotic mechanism inside the vacuum chamber reconfigures the distribution of tiny slits in the focal plane in under six minutes. Eight years in the making with First Light in 2012, MOSFIRE’s early performance results range from the discovery of ultra-cool, nearby substellar mass objects, to the detection of oxygen in young galaxies only two billion years after the Big Bang.
Other Authors
- UC Davis: Kuang-Han Huang, Brian Lemaux, and Julie He
- University of Melbourne, Australia: Michele Trenti and Stephanie Bernard
- University of California, Los Angeles (UCLA): Tommaso Treu, Louis E. Abramson, Charlotte Mason, and Takahiro Morishita
- Leibniz-Institut für Astrophysik Potsdam, Germany: Kasper Schmidt
- INAF Osservatorio Astronomico di Roma, Italy: Laura Pentericci
- Argelander-Institut für Astronomie, Bonn, Germany: Tim Schrabback
About W. M. Keck Observatory
The W. M. Keck Observatory operates the largest, most scientifically productive telescopes on Earth. The two, 10-meter optical/infrared telescopes on the summit of Maunakea on the Island of Hawaii feature a suite of advanced instruments including imagers, multi-object spectrographs, high-resolution spectrographs, an integral-field spectrometer and world-leading laser guide star adaptive optics systems. The Observatory is a private 501(c) 3 non-profit organization and a scientific partnership of the California Institute of Technology, the University of California, and NASA.
