New images from NASA's James Webb Space Telescope (JWST) have revealed that a well-known early galaxy has an overshadowed companion that is abundant with star formation.
A gravitationally lensed view of a ring-shaped slice of the galaxy SPT0418-47, as seen by the ALMA array in Chile. Recent observations by NASA's James Webb Space Telescope reveal that the galaxy has a satellite that's rich in star formation. (Image credit: ALMA (ESO/NAOJ/NRAO), Rizzo et al.)JWST's initial target was SPT0418-47, one of the brightest dusty, star-forming galaxies in the early universe. Given it is an extremely distant galaxy — it lies about 12 billion light-years from Earth — its light is bent and magnified by the gravity of another galaxy in the foreground (located between SPT0418-47 and the space telescope), creating a near perfect circle called an Einstein ring.
Using the JWST, astronomers were able to get a clearer view of SPT0418-47 and spotted a curious blob of light shining near the galaxy's outer edge. As it turns out, the blob represents a companion galaxy previously overshadowed by the light of the foreground galaxy, according to a statement from Cornell University.
"We found this galaxy to be super-chemically abundant, something none of us expected," Bo Peng, lead author of the study and a doctoral student in astronomy at Cornell, said in the statement. "JWST changes the way we view this system and opens up new venues to study how stars and galaxies formed in the early universe."
Earlier observations of SPT0418-47 using the Atacama Large Millimeter/submillimeter Array (ALMA) in Chile contained hints of the companion, which, at the time, were interpreted as random noise, the researchers said.
Using the JWST, the researcher discovered that the companion galaxy, called SPT0418-SE, is within about 16,000 light-years of SPT0418-47. By comparison, the Magellanic Clouds — a pair of dwarf galaxy companions to the Milky Way — are located roughly 160,000 light-years away from us.
The close proximity of SPT0418-47 and SPT0418-SE suggests these galaxies are bound to interact or merge with one another eventually. In turn, this galactic pair could shed light on how early galaxies evolved into larger ones, given SPT0418-47 is believed to have formed when the universe was only 1.4 billion years old, according to the statement.
Earlier observations of SPT0418-47 using the Atacama Large Millimeter/submillimeter Array (ALMA) in Chile contained hints of the companion, which, at the time, were interpreted as random noise, the researchers said.
Using the JWST, the researcher discovered that the companion galaxy, called SPT0418-SE, is within about 16,000 light-years of SPT0418-47. By comparison, the Magellanic Clouds — a pair of dwarf galaxy companions to the Milky Way — are located roughly 160,000 light-years away from us.
The close proximity of SPT0418-47 and SPT0418-SE suggests these galaxies are bound to interact or merge with one another eventually. In turn, this galactic pair could shed light on how early galaxies evolved into larger ones, given SPT0418-47 is believed to have formed when the universe was only 1.4 billion years old, according to the statement.
Interestingly, SPT0418-SE is believed to have already hosted multiple generations of stars, despite its young age. Both of the galaxies have a mature metallicity — or large amounts of elements like carbon, oxygen and nitrogen that are heavier than hydrogen and helium — which is similar to the sun. However, our sun is 4.5 billion years old and inherited most of its metals from previous generations of stars that were eight billion years old, the researchers said.
"We are seeing the leftovers of at least a couple of generations of stars having lived and died within the first billion years of the universe's existence, which is not what we typically see," study co-author Amit Vishwas, a research associate at the Cornell Center for Astrophysics and Planetary Sciences, said in the same statement.
"We speculate that the process of forming stars in these galaxies must have been very efficient and started very early in the universe, particularly to explain the measured abundance of nitrogen relative to oxygen, as this ratio is a reliable measure of how many generations of stars have lived and died," Vishwas said.
The new findings were published Feb. 17 in the Astrophysical Journal Letters.
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