View source for ID2299

{{Infobox astronomical event|name=ID2299|distance=9 billion light years|successor=|predecessor=|website=|energy=|peak=|notes=|b-v=|progenitor_type=|progenitor=|host=|remnant=|source=|redshift=|gal=|image=|epoch=|dec=|ra=|constellation=|detected_by=ALMA|duration=few minutes|start_time=11 January 2021|class=|event_type=observation|alt=|caption=|image_size=|commons=}}
'''ID2299''' is an [[elliptical galaxy]] 9 billion [[light-year]]s away.<ref name="ctvnews">{{cite web |url=https://www.ctvnews.ca/sci-tech/a-distant-galaxy-dies-as-astronomers-watch-1.5261943|title=A distant galaxy dies |author= Ashley Strickland|date=2021 |website=ctvnews.ca |access-date= 21 February 2021}}</ref><ref name="numerama">{{cite web |url=https://www.numerama.com/sciences/681675-pourquoi-certaines-galaxies-massives-de-lunivers-jeune-se-sont-elles-eteintes.html |title=Pourquoi certaines galaxies massive de l'Univers jeune see sont-elles éteintes? |author= Nelly Lesage |date=2021 |website=numerama.com|access-date= 21 February 2021}}{{In lang|fr}}</ref> It was found and detailed in January 2021, due to its phenomenon of catastrophic gas loss. This is due, unless the prolonged observations are inexplicably misleading or a poorly understood mechanism is at hand, to a [[galactic merger|catastrophic merger]] &ndash; prompting a secondary part of the galaxy that hosts rapid star formation. ID2299's high star formation rate is far outweighed by its ejection of gas. Its trailing tail has grown to approximately half of its size.  ID2299 is extrapolated to lose so much more gas that it will only remain [[active galaxy|active]] &ndash; capable of new star formation &ndash; for a few more tens of millions of years.

== Observation == 
This galaxy has been observed for the first time thanks to the [[Atacama Large Millimeter Array]] (ALMA) telescope, which is the biggest radio telescope worldwide,<ref name="franceculture">Le journal des sciences{{cite web |url=https://www.franceculture.fr/emissions/le-journal-des-sciences/le-journal-des-sciences-du-mardi-12-janvier-2021 |title=Les astronomes assistent à la mort d'une galaxie très lointaine pour la première fois |author=Natacha Triou |date=2021 |website=franceculture.fr |access-date=18 February 2021 }}{{In lang|fr}}</ref> in Chile, which scans the sky looking for distant variations in radiation.<ref name="leparisien">{{cite web |url=https://www.leparisien.fr/sciences/voici-une-galaxie-en-train-de-mourir-12-01-2021-32TKGRAW3ND3VK5WLS4XGIQUAU.php |title=Voici une galaxie en train de mourir |author=Gaël Lombart |date=2021 |website=leparisien.fr |access-date=18 February 2021 }}{{In lang|fr}}</ref> Astronomers observed an extreme instance of the "death" of a galaxy, by losing its gas.<ref>{{Cite web |date=2021-02-07 |title=First-Ever Galaxy's Death Caught on Human Eyes & What Does It Mean? - Deftyled |url=https://deftyled.com/first-ever-galaxys-death-caught-on-human-eyes-what-does-it-mean/ |access-date=2022-08-19 |website=deftyled.com |language=en-US}}</ref> An impression has been made by [[Martin Kornmesser]],<ref name="leparisien" /> a graphist at ESA (the [[European Space Agency]]). This represents, in intensified form, the [[visible spectrum|visible and near-visible wavelength]] corrollaries to the seen radiation, which cannot be picked up with present equipment due to great lengthening of wavelength ([[redshift]]). 
On 11 January 2021 the study was published in the journal ''[[Nature Astronomy]]''.<ref name="nature">{{cite journal |url=https://www.nature.com/articles/s41550-020-01268-x |title=A titanic interstellar medium ejection from a massive starburst galaxy at z=1.4 |author=Puglisi, A., Daddi, E., Brusa, M. and al. |date=2021 |website=nature.com| doi=10.1038/s41550-020-01268-x | arxiv=2101.04021 | s2cid=231573025 |access-date=18 February 2021}}</ref><ref name="ESO">{{cite web |url=https://www.eso.org/public/archives/releases/sciencepapers/eso2101/eso2101a.pdf |title=A titanic interstellar medium ejection from a massive starburst galaxy at z=1.4 |author=Puglisi, A., Daddi, E., Brusa, M. and al. |date=2021 |website=eso.org |access-date=18 February 2021}}</ref>

== Characteristics ==

=== Distance === 
The light from this galaxy is deemed to be 9 billion light-years from the Earth, having taken that time to reach the Earth. When astronomers observe ID2299, it is as it was 4.5 billion years ago,<ref name="leparisien" /> while it is extrapolated that it is now about 13 billion light years away.<ref name="bfmtv">BFMTV Sciences {{cite web |url=https://www.bfmtv.com/sciences/des-astronomes-observent-pour-la-premiere-fois-une-galaxie-lointaine-en-train-de-mourir_AD-202101120206.html |title=Des astronomes observant pour la première fois une galaxie en train de mourir |author=<!--Not stated--> |date=2021 |website=bfmtv.com|access-date=18 February 2021}}{{In lang|fr}}</ref>

=== Context ===
Deep space astronomic observations strongly imply around 2,000 billion galaxies exist or have existed, each on average composed of billions to hundreds of billions of stars.<ref name="radiocanada">{{cite web |url=https://ici.radio-canada.ca/nouvelle/808675/univers-galaxies-2000milliards |title=2000 milliards de galaxies dans l'Univers |author=Alain Labelle|date=2016 |website=ici.radio-canada.ca |access-date=18 February 2021}}{{In lang|fr}}</ref> Every galaxy has a key component of gas, which allows them to produce stars, and when all these die, and no more are creating, the galaxy will cease to exist. This can happens well before tens of billions of years if a galaxy becomes inactive such as by losing virtually all the interstellar gas.  Such a loss makes it impossible to create new stars. 

=== Composition ===
ID2299 is observed with extreme &ndash; and very likely total &ndash; gas loss underway, which it ejects as a tidal tail.<ref name="ESO" />  The 46% which forms the tail is being augmented at a rate of around {{val|10000|ul=solar mass}} per year.<ref name="sciencesetavenir">{{cite web |url=https://www.sciencesetavenir.fr/espace/univers/alma-observe-une-galaxie-lointaine-en-collision-en-train-de-mourir_150728 |title=ALMA observe une galaxie lointaine en collision en train de mourir |author=<!--Not stated--> |date=2021 |website=sciencesetavenir.fr |access-date=18 February 2021}}{{In lang|fr}}</ref> Within the other 54%, are intense zones of star production totalling about {{val|550|ul=solar mass}} per year. To compare, the Milky Way now births about {{val|3|ul=solar mass}} per year.<ref name="sciencesetavenir" /> If it continues at this rhythm, or similar, the galaxy has only a few tens of millions of years left for star production,<ref name="leparisien" /> a very minute fraction of cosmic history.

=== Explanation === 
Major gas loss had been modelled as likely either from stellar winds, from star formation<ref name="sciencesetavenir" /> or from relativistic jets and other ejections from the supermassive [[black hole]] and its sphere of influence, in the galactic nucleus. The accretion of matter there is accompanied by the emission of large amounts of energy and the appearance of powerful winds, capable of sweeping away the galaxy's gas.<ref name="lesechos">{{cite web |url=https://www.lesechos.fr/idees-debats/sciences-prospective/quand-les-galaxies-seteignent-1281524 |title=Quand les galaxies s'éteingnent |author=Yann Verdo |date=2021 |website=lesechos.fr |access-date=18 February 2021}}{{In lang|fr}}</ref> ID2299's data to a high probability presents to ESA scientists another mechanism: the collision of galaxies.<ref name="sciencesetavenir" /><ref>Scientific Paper (2021). https://www.almaobservatory.org/en/press-releases/alma-captures-distant-colliding-galaxy-dying-out-as-it-loses-the-ability-to-form-stars/.  Retrieved February 22, 2021</ref> Even if astronomers only observed the galaxy for few minutes,<ref name="ESO" /> they concluded that this tidal tail,<ref name="ESO" /> which will lead to the death of ID2299 is the result of a catastrophic collision between two galaxies, integral to the form and fate of ID2299.  In this earlier stage of the universe galaxies were closer together so more mergers took place, many dislodging high quantities of their respective [[interstellar medium|interstellar matter]].<ref name="franceculture" />

This catastrophic merger mechanism, if matched by very similar observations as the working group hypothesises it will be, has contributed to shape the make-up and distribution of the later surviving galaxies &ndash; including their host [[galaxy cluster]]s and [[galaxy supercluster|superclusters]] as we see in the more local universe.<ref name="sciencesetavenir" />

== References ==
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{{2021 in space}}
[[Category:Galaxies]]