Astronomy:MACS J1149 Lensed Star 1

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Short description: Blue supergiant and second most distant star from earth detected in the constellation Leo
MACS J1149 Lensed Star 1
NASA-Icarus-MostDistantMainSequenceStar-20180402.jpg
Detection of MACS J1149 Lensed Star 1
A galactic cluster (left) magnified a distant star (now named Icarus) more than 2,000 times, making it visible in 2016 from Earth (lower right), 9.34 billion light-years away—although visible in 2016, the star was not visible in 2011 (upper right).
Observation data
Equinox J2000.0]] (ICRS)
Constellation Leo[1][2]
Right ascension  11h 49m 35.59s[1]
Declination 22° 23′ 47.4″[1]
Astrometry
DistanceRedshift of 1.49 yields comoving distances of 14.4 billion ly
Characteristics
Spectral type B[2]
Apparent magnitude (V) ≈28.4[2] (normally 29.9)[note 1]
Apparent magnitude (R) ≈28.2[2] (normally 29.7)
Apparent magnitude (Z) ≈27.9[2] (normally 29.4)
Apparent magnitude (J) 27.3[2] (normally 28.8)
Apparent magnitude (H) 27.4[2] (normally 28.9)
Details
Surface gravity (log g)2 - 4[2] cgs
Temperature11,000 – 14,000[2] K
Metallicity≈0.006[2]
Age~8[2] Myr
Other designations
Icarus, LS1, MACS J1149 LS1, MACS J1149 Lensed Star 1 (LS1), MACS J1149+2223 Lensed Star 1

MACS J1149 Lensed Star 1, also known as Icarus,[note 2] is a blue supergiant star observed through a gravitational lens. It is the seventh most distant individual star to have been detected so far (after Earendel, Godzilla, Mothra, Quyllur, star-1 and star-2), at approximately 14 billion light-years from Earth (redshift z=1.49; comoving distance of 14.4 billion light-years; lookback time of 9.34 billion years).[3][2][4][5][6][7][8] Light from the star was emitted 4.4 billion years after the Big Bang.[7] According to co-discoverer Patrick Kelly, the star is at least a hundred times more distant than the next-farthest non-supernova star observed, SDSS J1229+1122, and is the first magnified individual star seen.[4][7]

History

Comparison of observed data of the star Icarus with a model of a blue supergiant star spectrum. Ultraviolet light is redshifted into the visible range and the star appears reddish.

In April and May 2018,[2] the star was found in the course of studying the supernova SN Refsdal with the Hubble Space Telescope. Astronomer Patrick Kelly of the University of Minnesota is the lead author of the finding, published in the journal Nature Astronomy.[2][8]

While astronomers had been collecting images of this supernova from 2004 onward, they recently discovered a point source that had appeared in their 2013 images, and become much brighter by 2016. They determined that the point source was a solitary star being magnified more than 2,000 times by gravitational lensing.[2][4][5][6][7][9] The light from LS1 was magnified not only by the huge total mass of the galaxy cluster MACS J1149+2223—located 5 billion light-years away—but also transiently by another compact object of about three solar masses within the galaxy cluster itself that passed through the line of sight, an effect known as gravitational microlensing.[7][9][10] The galaxy cluster magnification is probably a factor of 600, while the microlensing event, which peaked in May 2016, brightened the image by an additional factor of ~4.[2] There was a second peak near the brightness curve maximum, which may indicate the star was binary.[2] The microlensing body may have been a star or a black hole in the cluster. Continuous monitoring of the star Icarus may one day rule out the possibility that primordial black holes constitute a sizable fraction of dark matter.[9] Normally, the only astronomical objects that can be detected at this range would be either whole galaxies, quasars, or supernovas, but the light from the star was magnified by the lensing effect. They determined the light was from a stable star, not a supernova, as its temperature did not fluctuate; the temperature also allowed them to catalog the star as a blue supergiant.[11] Because the visible light is the redshifted ultraviolet tail, the star does not appear blue to us but reddish or pink.

The light observed from the star was emitted when the universe was about 30% of its current age of 13.8 billion years. Kelly suggested that similar microlensing discoveries could help them identify the earliest stars in the universe.[11]

Name

The formal name MACS J1149 is a reference to MAssive Cluster Survey and the star's coordinates in the J2000 astronomical epoch.

While Kelly had wanted to name the star Warhol, alluding to Andy Warhol's notion of having 15 minutes of fame, the team ended up naming the star Icarus based on the Greek mythological figure.[8]

Astrophysical implications

The discovery shows that astronomers can study the oldest stars in background galaxies of the early universe by combining the strong gravitational lensing effect from galaxy clusters with gravitational microlensing events caused by compact objects in these galaxy clusters.[2][12] By using these events, astronomers can study and test some models about dark matter in galaxy clusters and observe high energy events (supernovae, variable stars) in young galaxies.[9][12][13]

See also

Notes

  1. ↑ The microlensing event brightened the star by a factor of 4, or about 1.5 magnitudes. With 600× magnification, it is brightened by 6002 (360,000), which would be an additional magnitude difference of 13.9 magnitudes. Therefore, the star would have Vmag of 43.8 without any lensing effects, thousands of times dimmer than any current or planned telescopes can see.
  2. ↑ Other names include LS1, MACS J1149 LS1, MACS J1149 Lensed Star 1 (LS1) and MACS J1149+2223 Lensed Star 1

References

  1. ↑ 1.0 1.1 1.2 1.3 Kelly, P. L. (2015). "Multiple images of a highly magnified supernova formed by an early-type cluster galaxy lens". Science 347 (6226): 1123–1126. doi:10.1126/science.aaa3350. PMID 25745167. Bibcode: 2015Sci...347.1123K. 
  2. ↑ 2.00 2.01 2.02 2.03 2.04 2.05 2.06 2.07 2.08 2.09 2.10 2.11 2.12 2.13 2.14 2.15 2.16 2.17 Kelly, Patrick L. (2 April 2018). "Extreme magnification of an individual star at redshift 1.5 by a galaxy-cluster lens". Nature Astronomy 2 (4): 334–342. doi:10.1038/s41550-018-0430-3. Bibcode: 2018NatAs...2..334K. 
  3. ↑ Staff (2018). "Cosmological information and results: redshift z=1.49". Wolfram Alpha. http://www.wolframalpha.com/input/?i=redshift+z%3D1.49&a=FSelect_**LookbackTimeFromRedshift--. 
  4. ↑ 4.0 4.1 4.2 Jenkins, Ann; Villard, Ray; Kelly, Patrick (2 April 2018). "Hubble Uncovers the Farthest Star Ever Seen". NASA. https://www.nasa.gov/feature/goddard/2018/hubble-uncovers-the-farthest-star-ever-seen. 
  5. ↑ 5.0 5.1 Howell, Elizabeth (2 April 2018). "Rare Cosmic Alignment Reveals Most Distant Star Ever Seen". Space.com. https://www.space.com/40171-cosmic-alignment-reveals-most-distant-star-yet.html. 
  6. ↑ 6.0 6.1 Sanders, Robert (2 April 2018). "Hubble peers through cosmic lens to capture most distant star ever seen". Berkeley News. http://news.berkeley.edu/2018/04/02/cosmic-lens-helps-hubble-capture-most-distant-star-ever-seen/. 
  7. ↑ 7.0 7.1 7.2 7.3 7.4 Parks, Jake (2 April 2018). "Hubble spots farthest star ever seen". Astronomy. http://www.astronomy.com/news/2018/04/hubble-images-farthest-star-ever-seen. 
  8. ↑ 8.0 8.1 8.2 Dunham, Will (2 April 2018). "Most distant star ever detected sits halfway across the universe". Reuters. https://www.reuters.com/article/us-space-icarus/most-distant-star-ever-detected-sits-halfway-across-the-universe-idUSKCN1H921F. 
  9. ↑ 9.0 9.1 9.2 9.3 Diego, J.M. (2 April 2018). "Dark Matter Under the Microscope: Constraining compact dark matter with caustic crossing events". The Astrophysical Journal 857 (1): 25. doi:10.3847/1538-4357/aab617. Bibcode: 2018ApJ...857...25D. 
  10. ↑ "Hubble uses cosmic lens to discover most distant star ever observed". 2 April 2018. http://spacetelescope.org/news/heic1807/. 
  11. ↑ 11.0 11.1 Guarino, Ben (3 April 2018). "This star is the farthest ever seen. It's 9 billion light-years away". The Washington Post. https://www.washingtonpost.com/news/speaking-of-science/wp/2018/04/03/this-star-is-the-farthest-ever-seen-its-9-billion-light-years-away/. 
  12. ↑ 12.0 12.1 Rosanne Di Stefano (2 April 2018). "Cosmic flashing lights". Nature Astronomy. https://www.nature.com/articles/s41550-018-0416-1. 
  13. ↑ S. A. Rodney (2 April 2018). "Two peculiar fast transients in a strongly lensed host galaxy". Nature Astronomy 2 (4): 324–333. doi:10.1038/s41550-018-0405-4. Bibcode: 2018NatAs...2..324R. 

External links



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