List of most distant stars

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This is a list of the most distant individually seen stars discovered.

List

List of most distant individually seen stars
StarRedshiftDistance (Mpc)DiscoveryNotes
WHL0137-LS (Earendel)6.2±0.1 [1] 8,6002022The most distant known star as of 2023.
MACS J0647.7+7015 LS14.8 [2] 7,8302023
MACS J0647.7+7015 LS2
Abell 2744 LS12.65 [3] 6,1102022
Godzilla 2.38 [4] 5,7802022The most luminous known star.
Quyllur 2.1878 [5] 5,5402023First red supergiant at cosmological distances.
Mothra 2.091 [6] 5,4002023A binary consisting of a yellow supergiant or yellow hypergiant and a Blue supergiant.
MACS J1149 Lensed Star 1 1.49 [7] 4,4102018The most distant known star prior to the discovery of Earendel.
Warhol0.94 [8] 3,0002014Transient, extremely luminous O-type star or a Large Wolf-Rayet star [9]
AT 2022zmn 0.019 [10] 842022 Luminous blue variable.
AT 2022oku 0.018 [11] 792022 Luminous blue variable.
AT 2018kle 0.012505 [12] 552018 Luminous blue variable.
SDSS J1229+1122 0.00012717
[ clarification needed ]
2013 Blue supergiant.

Related Research Articles

<span class="mw-page-title-main">Blue supergiant</span> Hot, luminous star with a spectral type of A9 or earlier

A blue supergiant (BSG) is a hot, luminous star, often referred to as an OB supergiant. They are usually considered to be those with luminosity class I and spectral class B9 or earlier, although sometimes A-class supergiants are also deemed blue supergiants.

<span class="mw-page-title-main">Reionization</span> Process that caused matter to reionize early in the history of the Universe

In the fields of Big Bang theory and cosmology, reionization is the process that caused electrically neutral atoms in the universe to reionize after the lapse of the "dark ages".

<span class="mw-page-title-main">GQ Lupi b</span> Exoplanet candidate orbiting GQ Lupi. Either a brown dwarf or exoplanet.

GQ Lupi b, or GQ Lupi B, is a possible extrasolar planet, brown dwarf or sub-brown dwarf orbiting the star GQ Lupi. Its discovery was announced in April 2005, less than a month before the full confirmation of 2M1207b was announced. Along with 2M1207b, this was one of the first extrasolar planet candidates to be directly imaged. The image was made with the European Southern Observatory's VLT telescope at the Paranal Observatory, Chile on June 25, 2004.

<span class="mw-page-title-main">Yellow hypergiant</span> Class of massive star with a spectral type of A to K

A yellow hypergiant (YHG) is a massive star with an extended atmosphere, a spectral class from A to K, and, starting with an initial mass of about 20–60 solar masses, has lost as much as half that mass. They are amongst the most visually luminous stars, with absolute magnitude (MV) around −9, but also one of the rarest, with just 20 known in the Milky Way and six of those in just a single cluster. They are sometimes referred to as cool hypergiants in comparison with O- and B-type stars, and sometimes as warm hypergiants in comparison with red supergiants.

<span class="mw-page-title-main">Galaxy filament</span> Largest structures in the universe, made of galaxies

In cosmology, galaxy filaments are the largest known structures in the universe, consisting of walls of galactic superclusters. These massive, thread-like formations can commonly reach 50/h to 80/h megaparsecs —with the largest found to date being the Hercules-Corona Borealis Great Wall at around 3 gigaparsecs (9.8 Gly) in length—and form the boundaries between voids. Due to the accelerating expansion of the universe, the individual clusters of gravitationally bound galaxies that make up galaxy filaments are moving away from each other at an accelerated rate; in the far future they will dissolve.

<span class="mw-page-title-main">MACS0647-JD</span> One of the farthest known galaxies from the Earth in the constellation Camelopardalis

MACS0647-JD is a galaxy with a redshift of about z = 10.7, equivalent to a light travel distance of 13.26 billion light-years. If the distance estimate is correct, it formed about 427 million years after the Big Bang.

<span class="mw-page-title-main">MACS J0647.7+7015</span> Galaxy cluster in the constellation Camelopardalis

MACS J0647.7+7015 is a galaxy cluster with a redshift z = 0.592, located at J2000.0 right ascension 06h 47m 42s declination +70° 15′. It lies between the Big Dipper and Little Dipper in the constellation Camelopardalis. It is part of a sample of 12 extreme galaxy clusters at z > 0.5 discovered by the MAssive Cluster Survey (MACS).

<span class="mw-page-title-main">SN Refsdal</span> Supernova that has been lensed

SN Refsdal is the first detected multiply-lensed supernova, visible within the field of the galaxy cluster MACS J1149+2223. It was named after Norwegian astrophysicist Sjur Refsdal, who, in 1964, first proposed using time-delayed images from a lensed supernova to study the expansion of the universe. The observations were made using the Hubble Space Telescope.

<span class="mw-page-title-main">Circumplanetary disk</span> Accumulation of matter around a planet

A circumplanetary disk is a torus, pancake or ring-shaped accumulation of matter composed of gas, dust, planetesimals, asteroids or collision fragments in orbit around a planet. They are reservoirs of material out of which moons may form. Such a disk can manifest itself in various ways.

<span class="mw-page-title-main">WHL0137-LS</span> Most distant known star, discovered 2022

WHL0137-LS, also known as Earendel, is a star located in the constellation of Cetus. Discovered in 2022 by the Hubble Space Telescope, it is the earliest and most distant known star, at a comoving distance of 28 billion light-years. The previous farthest known star, MACS J1149 Lensed Star 1, also known as Icarus, at a comoving distance of 14.4 billion light-years, was discovered by Hubble in 2018. Stars like Earendel can be observed at cosmological distances thanks to the large magnification factors afforded by gravitational lensing, which can exceed 1,000. Other stars have been observed through this technique, such as Godzilla.

<span class="mw-page-title-main">Godzilla (star)</span> Star in the Sunburst galaxy

Godzilla is a variable star in the Sunburst galaxy at redshift z = 2.37, observed through the gravitational lens PSZ1 G311.65-18.48. It was originally identified in the NW arc as a possible transient event in images taken with the Hubble Space Telescope (HST).

<span class="mw-page-title-main">Sunburst galaxy</span> Galaxy

The Sunburst galaxy is a strongly magnified galaxy at redshift z=2.38 behind the galaxy cluster PSZ1 G311.65-18.48.

<span class="mw-page-title-main">UNCOVER-z13</span> High-redshift galaxy in Sculptor constellation

UNCOVER-z13 is a high-redshift Lyman-break galaxy discovered by the James Webb Space Telescope (JWST) during NIRCam imaging for the JWST Ultradeep NIRSpec and NIRCam Observations before the Epoch of Reionization (UNCOVER) project on November 14, 2023. UNCOVER-z13 is within Abell 2744 supercluster in the constellation Sculptor.

<span class="mw-page-title-main">UNCOVER-z12</span> Lyman-break galaxy in the constellation Sculptor

UNCOVER-z12 is a high-redshift Lyman-break galaxy discovered by the James Webb Space Telescope (JWST) during NIRCam imaging for the JWST Ultradeep NIRSpec and NIRCam Observations before the Epoch of Reionization (UNCOVER) project in November 2023. UNCOVER-z12 is within the Abell 2744 supercluster in the constellation Sculptor. It is the 5th-most distant object ever discovered as of 2024, and is estimated to be 32.21 giga-lightyears from Earth.

Mothra, or EMO J041608.838-240358.60, is a binary system with a possible transient, in the constellation of Eridanus. Mothra is in the galaxy cluster MACS J0416.1-2403, nicknamed the "Christmas Tree Galaxy Cluster".

<span class="mw-page-title-main">UNCOVER-BD-1</span> UNCOVER-BD-1 is a distant brown dwarf

UNCOVER-BD-1 is a distant brown dwarf. It is the most distant T dwarf discovered to date.

References

  1. Welch, Brian; Coe, Dan; Diego, Jose M.; Zitrin, Adi; Zackrisson, Erik; Dimauro, Paola; Jiménez-Teja, Yolanda; Kelly, Patrick; Mahler, Guillaume; Oguri, Masamune; Timmes, F. X.; Windhorst, Rogier; Florian, Michael; de Mink, S. E.; Avila, Roberto J. (March 2023). "A highly magnified star at redshift 6.2". Nature. 603 (7903): 815–818. arXiv: 2209.14866 . doi:10.1038/s41586-022-04449-y. ISSN   1476-4687. PMID   35354998. S2CID   247842625.
  2. Meena, Ashish Kumar; Zitrin, Adi; Jiménez-Teja, Yolanda; Zackrisson, Erik; Chen, Wenlei; Coe, Dan; Diego, Jose M.; Dimauro, Paola; Furtak, Lukas J.; Kelly, Patrick L.; Oguri, Masamune; Welch, Brian; Abdurro’uf; Andrade-Santos, Felipe; Adamo, Angela (February 2023). "Two Lensed Star Candidates at z ≃ 4.8 behind the Galaxy Cluster MACS J0647.7+7015". The Astrophysical Journal Letters. 944 (1): L6. arXiv: 2211.13334 . Bibcode:2023ApJ...944L...6M. doi: 10.3847/2041-8213/acb645 . hdl: 10810/61038 . ISSN   2041-8205.
  3. Chen, Wenlei; Kelly, Patrick L.; Treu, Tommaso; Wang, Xin; Roberts-Borsani, Guido; Keen, Allison; Windhorst, Rogier A.; Zhou, Rui; Bradac, Marusa; Brammer, Gabriel; Strait, Victoria; Broadhurst, Tom J.; Diego, Jose M.; Frye, Brenda L.; Meena, Ashish K. (1 December 2022). "Early Results from GLASS-JWST. VIII. An Extremely Magnified Blue Supergiant Star at Redshift 2.65 in the A2744 Cluster Field". The Astrophysical Journal Letters. 940 (2): L54. arXiv: 2207.11658 . Bibcode:2022ApJ...940L..54C. doi: 10.3847/2041-8213/ac9585 . hdl: 10810/59535 . ISSN   2041-8205.
  4. Diego, J. M.; Pascale, M.; Kavanagh, B. J.; Kelly, P.; Dai, L.; Frye, B.; Broadhurst, T. (1 September 2022). "Godzilla, a monster lurks in the Sunburst galaxy". Astronomy & Astrophysics. 665: A134. arXiv: 2203.08158 . Bibcode:2022A&A...665A.134D. doi: 10.1051/0004-6361/202243605 . ISSN   0004-6361. S2CID   247476158.
  5. Diego, J. M.; Meena, A. K.; Adams, N. J.; Broadhurst, T.; Dai, L.; Coe, D.; Frye, B.; Kelly, P.; Koekemoer, A. M.; Pascale, M.; Willner, S. P.; Zackrisson, E.; Zitrin, A.; Windhorst, R. A.; Cohen, S. H. (1 April 2023). "JWST's PEARLS: A new lens model for ACT-CL J0102−4915, "El Gordo," and the first red supergiant star at cosmological distances discovered by JWST". Astronomy and Astrophysics. 672: A3. arXiv: 2210.06514 . Bibcode:2023A&A...672A...3D. doi:10.1051/0004-6361/202245238. ISSN   0004-6361. S2CID   252873244.
  6. Diego, Jose M.; Sun, Bangzheng; Yan, Haojing; Furtak, Lukas J.; Zackrisson, Erik; Dai, Liang; Kelly, Patrick; Nonino, Mario; Adams, Nathan; Meena, Ashish K.; Willner, Steven P.; Zitrin, Adi; Cohen, Seth H.; D’Silva, Jordan C. J.; Jansen, Rolf A. (1 November 2023). "JWST's PEARLS: Mothra, a new kaiju star at z = 2.091 extremely magnified by MACS0416, and implications for dark matter models". Astronomy & Astrophysics. 679: A31. arXiv: 2307.10363 . Bibcode:2023A&A...679A..31D. doi: 10.1051/0004-6361/202347556 . ISSN   0004-6361. S2CID   259991552.
  7. Kelly, Patrick L.; Diego, Jose M.; Rodney, Steven; Kaiser, Nick; Broadhurst, Tom; Zitrin, Adi; Treu, Tommaso; Pérez-González, Pablo G.; Morishita, Takahiro; Jauzac, Mathilde; Selsing, Jonatan; Oguri, Masamune; Pueyo, Laurent; Ross, Timothy W.; Filippenko, Alexei V. (April 2018). "Extreme magnification of an individual star at redshift 1.5 by a galaxy-cluster lens". Nature Astronomy. 2 (4): 334–342. arXiv: 1706.10279 . Bibcode:2018NatAs...2..334K. doi:10.1038/s41550-018-0430-3. ISSN   2397-3366. S2CID   256703331.
  8. Chen, Wenlei (2019). "Searching for Highly Magnified Stars at Cosmological Distances: Discovery of a Redshift 0.94 Blue Supergiant in Archival Images of the Galaxy Cluster MACS J0416.1-2403". arXiv: 1902.05510 [astrophysics].
  9. https://iopscience.iop.org/article/10.3847/1538-4357/ab297d
  10. "AT 2020zmn". Transient Name Server. IAU . Retrieved 30 August 2024.
  11. "AT 2022oku". Transient Name Server. IAU . Retrieved 29 August 2024.
  12. "AT 2018kle". Transient Name Server. IAU . Retrieved 30 August 2024.