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SPT 0346-52: Under Construction: Distant Galaxy Churning Out Stars at Remarkable Rate
SPT 0346-52

  • SPT0346-52 is a galaxy found about a billion years after the Big Bang that has one of the highest rates of star formation ever seen in a galaxy.

  • Astronomers discovered this stellar construction boom by combining data from Chandra and several other telescopes.

  • ALMA revealed this galaxy gave off extreme amount of infrared emission, which could have multiple explanations.

  • Chandra's observations ruled out the presence of an actively growing supermassive black hole, bolstering the case of extreme star formation in this galaxy.

This graphic shows a frame from a computer simulation (main image) and astronomical data (inset) of a distant galaxy undergoing an extraordinary construction boom of star formation, as described in our press release. The galaxy, known as SPT0346-52, is 12.7 billion light years from Earth. This means that astronomers are observing it at a critical stage in the evolution of galaxies, about a billion years after the Big Bang.

Astronomers were intrigued by SPT0346-52 when data from the Atacama Large Millimeter/submillimeter Array (ALMA) revealed extremely bright infrared emission from this galaxy. This suggested that the galaxy is undergoing a tremendous explosion of star birth.

However, another possible explanation for the excess infrared emission was the presence of a rapidly growing supermassive black hole at the galaxy's center. In this scenario, gas falling towards the black hole would become much hotter and brighter, causing surrounding dust and gas to glow in infrared light.

To distinguish between these two possibilities, researchers used NASA's Chandra X-ray Observatory and CSIRO's Australia Telescope Compact Array (ATCA), a radio telescope. Neither X-rays nor radio waves were detected, so astronomers were able to rule out a growing black hole generating most of the bright infrared light. Therefore, they determined that SPT0346-52 is undergoing a tremendous amount of star formation, an important discovery for a galaxy found so early in the Universe.

The main panel of the graphic shows one frame of a simulation produced on a supercomputer. The distorted galaxy shown here results from a collision between two galaxies followed by them merging. Astronomers think such a merger could be the reason why SPT0346-52 is having such a boom of stellar construction. Once the two galaxies collide, gas near the center of the merged galaxy (shown as the bright region in the center of the simulation) is compressed, producing the burst of new stars seen forming in SPT0346-52. The dark regions in the simulation represent cosmic dust that absorbs and scatters starlight.

Labeled
Labeled

The inset in this graphic contains a composite image with X-ray data from Chandra (blue), short wavelength infrared data from Hubble (green), infrared light from Spitzer (red) at longer wavelengths, and infrared data from ALMA (magenta) at even longer wavelengths. In the latter case the light from SPT0346-52 is distorted and magnified by the gravity of an intervening galaxy, producing three elongated images in the ALMA data located near the center of the image. SPT0346-52 is not visible in the Hubble or Spitzer data, but the intervening galaxy causing the gravitational lensing is detected. The bright galaxy seen in the Hubble and Spitzer data slightly to the left of the image's center is unrelated to SPT0346-52.

There is no blue at the center of the image, showing that Chandra did not detect any X-rays that could have signaled the presence of a growing black hole. The ATCA data, not shown here, also involved the non-detection of a growing black hole. These data suggest that SPT0346-52 is forming at a rate of about 4,500 times the mass of the Sun every year, one of the highest rates seen in a galaxy. This is in contrast to a galaxy like the Milky Way that only forms about one solar mass of new stars per year.

A paper describing these results, with first author Jingzhe Ma (University of Florida), has been accepted for publication in The Astrophysical Journal and is available online. NASA's Marshall Space Flight Center in Huntsville, Alabama, manages the Chandra program for NASA's Science Mission Directorate in Washington. The Smithsonian Astrophysical Observatory in Cambridge, Massachusetts, controls Chandra's science and flight operations.

Fast Facts for SPT 0346-52:
Credit  X-ray: NASA/CXC/Univ of Florida/J.Ma et al; Optical: NASA/STScI; Infrared: NASA/JPL-Caltech; Radio: ESO/NAOJ/NRAO/ALMA; Simulation: Simons Fdn./Moore Fdn./Flatiron Inst./Caltech/C. Hayward & P. Hopkins
Release Date  December 8, 2016
Scale  Image is 46 arcsec across (about 900,000 light years)
Category  Normal Galaxies & Starburst Galaxies
Coordinates (J2000)  RA 03h 46m 41.13s | Dec -52 05' 02.11"
Constellation  Horologium
Observation Date  29 Jul 2015
Observation Time  13 hours 53 min.
Obs. ID  17132
Instrument  ACIS
References Ma, J. et al, 2016, ApJ (accepted); arXiv:1609.08553
Color Code  X-ray (Blue), Optical (Green), Infrared (Red), Radio (Purple)
Radio
IR
Optical
X-ray
Distance Estimate  About 12.7 billion light years (z=5.656)
distance arrow
Visitor Comments (3)

How wonderful, I've always enjoyed the images that show up on my email program.
How do I get my grandchildren involved with the same?

Posted by Stephen Gordon on Thursday, 01.12.17 @ 23:48pm


It is incredible to see such a distant object from wildly different perspectives, all from one vantage point that uses another massive object very far away as a mean to peer in on the otherwise-hidden object from different angles. Almost unreal to come to terms with in one's head...
It's 2016 right, Not 3016

Posted by Ben on Friday, 12.9.16 @ 21:48pm


What are the two green ovals, slightly to the left and above the lensed images of SPT 0346-52, and the round bright magenta spot in the upper left corner, are these galaxies unrelated to the SPT 0346-52? Thanks

Posted by Bondybey on Friday, 12.9.16 @ 10:06am


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