Z8 GND 5296

{{Short description|Dwarf galaxy}}

{{DISPLAYTITLE:z8_GND_5296}}

{{Infobox galaxy

| name = z8_GND_5296

| image = Z8 GND 5296.jpg

| caption = z8_GND_5296 image from the NASA/ESA Hubble Space Telescope in 2013

| epoch = J2000

| constellation name = Ursa Major

| ra = {{RA|12|36|37.892}}

| dec = {{DEC|+62|18|08.54}}

| z = {{val|7.5078|0.0004}}

| h_radial_v = {{val|291622|120|ul=km/s}}

| gal_v =

| dist_ly = {{nowrap| {{convert|13.1|e9ly|e9pc|abbr=unit|lk=on}} }}
(light travel distance)
≈{{convert|30|e9ly|e9pc|abbr=unit}}
{{nowrap|(present comoving distance)}}

| type = Dwarf

| mass = {{val|1.0|0.2|0.1|e=9}}

| size =

| stars =

| appmag_v = 25.6 (F160W)

| appmag_b =

| absmag_v =

| names = {{nowrap|FIGS GN1 1292}}, {{nowrap|J123637.89+621808.5}}, {{nowrap|z7 GND 42912}}

| references = {{cite journal |title=A galaxy rapidly forming stars 700 million years after the Big Bang at redshift 7.51 |journal=Nature |first1=S. L. |last1=Finkelstein |first2=C. |last2=Papovich |first3=M. |last3=Dickinson |first4=M. |last4=Song |first5=V. |last5=Tilvi |first6=A. M. |last6=Koekemoer |first7=K. D. |last7=Finkelstein |first8=B. |last8=Mobasher |first9=H. C. |last9=Ferguson |first10=M. |last10=Giavalisco |first11=N. |last11=Reddy |first12=M. L. N. |last12=Ashby |first13=A. |last13=Dekel |first14=G. G. |last14=Fazio |first15=A. |last15=Fontana |first16=N. A. |last16=Grogin |first17=J.-S. |last17=Huang |first18=D. |last18=Kocevski |first19=M. |last19=Rafelski |first20=B. J. |last20=Weiner |first21=S. P. |last21=Willner |display-authors=5 |volume=502 |issue=7472 |pages=524–527 |year=2013 |arxiv=1310.6031 |doi=10.1038/nature12657|bibcode = 2013Natur.502..524F |pmid=24153304|s2cid=4448085 }}{{cite simbad |title=NAME FIGS GN1 1292 |access-date=6 October 2016}}

}}

z8_GND_5296 is a dwarf galaxy{{cite news |url=https://www.washingtonpost.com/national/health-science/newly-detected-galaxy-is-the-most-distant-ever/2013/10/23/415ac854-3a78-11e3-b7ba-503fb5822c3e_story.html |title=Newly identified galaxy is the most distant ever confirmed |newspaper=The Washington Post |first=Meeri |last=Kim |date=23 October 2013 |access-date=22 October 2014}} discovered in October 2013 which has the highest redshift that has been confirmed through the Lyman-alpha emission line of hydrogen, placing it among the oldest and most distant known galaxies at approximately {{convert|13.1|e9ly|Gpc|}} from Earth.{{cite news |url=http://www.readthehorn.com/news/research/85364/farthest_galaxy_ever_seen_discovered_by_ut_researchers |title=Farthest galaxy ever seen discovered by UT researchers |work=The Horn |first=Mihir |last=Shukla |date=26 October 2013 |access-date=30 October 2013 |archive-date=30 October 2013 |archive-url=https://web.archive.org/web/20131030074352/http://www.readthehorn.com/news/research/85364/farthest_galaxy_ever_seen_discovered_by_ut_researchers |url-status=dead }}{{cite news |url=http://www.universetoday.com/105694/taking-measure-a-new-most-distant-galaxy/ |title=Taking Measure: A 'New' Most Distant Galaxy |work=Universe Today |first=Matthew |last=Francis |date=23 October 2013 |access-date=30 October 2013}} It is "seen as it was at a time just 700 million years after the Big Bang [...] when the universe was only about 5 percent of its current age of 13.8 billion years".{{cite press release |url=http://www.utexas.edu/news/2013/10/23/texas-astronomer-discovers-most-distant-known-galaxy/ |title=Texas Astronomer Discovers Most Distant Known Galaxy |publisher=University of Texas at Austin |first=Rebecca |last=Johnson |date=23 October 2013}} The galaxy is at a redshift of 7.51, and it is a neighbour to what was announced then as the second-most distant galaxy with a redshift of 7.2. The galaxy in its observable timeframe was producing stars at a phenomenal rate, equivalent in mass to about 330 Suns per year.

The light reaching Earth from z8_GND_5296 shows its position over 13 billion years ago, having traveled a distance of more than 13 billion light-years. Due to the expansion of the universe, this position is now at about {{convert|30|e9ly|Gpc}} (comoving distance) from Earth.{{cite news |url=https://www.bbc.co.uk/news/science-environment-24637890 |title=New galaxy 'most distant' yet discovered |work=BBC News |first=Rebecca |last=Morelle |author-link=Rebecca Morelle |date=23 October 2013 |access-date=24 October 2013}}

Discovery

File:KeckTelescopes-hi.png atop Mauna Kea in Hawaii]]

Research published in the 24 October 2013 issue of the journal Nature by a team of astronomers from the University of Texas at Austin led by Steven Finkelstein, in collaboration with astronomers at the Texas A&M University, the National Optical Astronomy Observatory and University of California, Riverside, describes the discovery of the most distant galaxy known using deep optical and infrared images taken by the Hubble Space Telescope. Their discovery was confirmed by the W. M. Keck Observatory in Hawaii. MOSFIRE, a new instrument at the Keck Observatory that is extremely sensitive to infrared light, proved instrumental to this finding.{{cite news |url=http://ucrtoday.ucr.edu/18589 |title=UC Riverside Astronomers Help Discover the Most Distant Known Galaxy |work=UCR Today |publisher=University of California, Riverside |first=Iqbal |last=Pittalwala |date=23 October 2013 |access-date=26 May 2014}}

To measure galaxies at such large distances with definitive evidence, astronomers use spectroscopy and the phenomenon of redshift. Redshift occurs whenever a light source moves away from an observer. Astronomical redshift is seen due to the expansion of the universe, and sufficiently distant light sources (generally more than a few million light-years away) show redshift corresponding to the rate of increase in their distance from Earth. The redshift observed in astronomy can be measured because the emission and absorption spectra for atoms are distinctive and well known, calibrated from spectroscopic experiments in laboratories on Earth.{{cite journal |title=Photometric Redshifts based on standard SED fitting procedures |journal=Astronomy and Astrophysics |first1=Micol |last1=Bolzonella |first2=Joan-Marc |last2=Miralles |first3=Roser |last3=Pelló |volume=363 |pages=476–492 |date=November 2000 |arxiv=astro-ph/0003380 |bibcode=2000A&A...363..476B}}

See also

References

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{{Galaxy}}

{{2013 in space}}

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20131012

Category:Dwarf galaxies

Category:Starburst galaxies

Category:Ursa Major

Category:Articles with underscores in the title