Astronomers set a new galaxy distance record

A team discovered an exceptionally luminous galaxy more than 13 billion years in the past; it existed so long ago that it appears to be only 100 million years old.
By and | Published: May 5, 2015 | Last updated on May 18, 2023

Distant galaxy
This is a Hubble Space Telescope image of the farthest spectroscopically confirmed galaxy observed to date (inset). It was identified in this Hubble image of a field of galaxies in the CANDELS survey (Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey). NASA’s Spitzer Space Telescope also observed the unique galaxy. The W. M. Keck Observatory was used to obtain a spectroscopic redshift (z=7.7), extending the previous redshift record. Measurements of the stretching of light, or redshift, give the most reliable distances to other galaxies. This source is thus currently the most distant confirmed galaxy known, and it appears to also be one of the brightest and most massive sources at that time. The galaxy existed over 13 billion years ago. The near-infrared light image of the galaxy (inset) has been colored blue as suggestive of its young, and hence very blue, stars. The CANDELS field is a combination of visible-light and near-infrared exposures.
NASA/ESA/P. Oesch (Yale Univ.)
An international team of astronomers, led by Yale University and University of California scientists, pushed back the cosmic frontier of galaxy exploration to a time when the universe was only 5 percent of its present age of 13.8 billion years. The team discovered an exceptionally luminous galaxy more than 13 billion years in the past and determined its exact distance from Earth using the combined data from NASA’s Hubble and Spitzer space telescopes and the Keck I 10-meter telescope at the W. M. Keck Observatory in Hawaii. These observations confirmed it to be the most distant galaxy currently measured, setting a new record. The galaxy existed so long ago, it appears to be only 100 million years old.

The galaxy EGS-zs8-1 was originally identified based on its particular colors in images from Hubble and Spitzer and is one of the brightest and most massive objects in the early universe. “It has already grown more than 15 percent of the mass of our own Milky Way today,” said Pascal Oesch from Yale University, New Haven, Connecticut. “But it had only 670 million years to do so. The universe was still very young then.” The new distance measurement also enabled the astronomers to determine that EGS-zs8-1 was still forming stars rapidly, about 80 times faster than the Milky Way Galaxy today, which has a star formation rate of one star per year.

HubbleAnniversary2
Only a handful of galaxies currently have accurate distances measured in this early universe. “Every confirmation adds another piece to the puzzle of how the first generations of galaxies formed in the early universe,” said Pieter van Dokkum of Yale. “Only the most sensitive telescopes are powerful enough to reach to these large distances.” The discovery was only possible thanks to the relatively new Multi-Object Spectrometer For Infra-Red Exploration (MOSFIRE) instrument on the Keck I Telescope, which allows astronomers to efficiently study several galaxies at the same time.

Measuring galaxies at these extreme distances and characterizing their properties is a main goal of astronomers over the next decade. The observations see EGS-zs8-1 at a time when the universe was undergoing important changes: The hydrogen between galaxies was transitioning from an opaque to a transparent state. “It appears that the young stars in the early galaxies like EGS-zs8-1 were the main drivers for this transition called reionization,” said Rychard Bouwens of the Leiden Observatory in the
Netherlands.

These new Hubble, Spitzer, and Keck observations together give a new glimpse into the nature of the infant universe. They confirm that massive galaxies already existed early in the history of the universe, but that their physical properties were different from galaxies seen around us today. Astronomers now have strong evidence that the peculiar colors of early galaxies seen in the Spitzer images originate from a rapid formation of massive, young stars, which interacted with the primordial gas in these galaxies.

The new observations underline the exciting discoveries that NASA’s James Webb Space Telescope will enable when it is launched in 2018. In addition to pushing the cosmic frontier to even earlier cosmic times, the Webb telescope will be able to dissect the infrared galaxy light of EGS-zs8-1 seen with the Spitzer Space Telescope and will provide astronomers with much more detailed insights into its gas properties. “Our current observations indicate that it will be easy to measure accurate distances to these distant galaxies in the future with the James Webb Space Telescope,” said Garth Illingworth of the University of California, Santa Cruz. “The result of Webb’s upcoming measurements will provide a much more complete picture of the formation of galaxies at the cosmic dawn.”