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Historical brightest stars

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This article'sfactual accuracy may be compromised due to out-of-date information. The reason given is:The results were produced before the new reduction ofHipparcos data (van Leeuwen, 2007) and theGaia mission. Please help update this article to reflect recent events or newly available information.(December 2017)

TheSolar System and all of the visible stars are in different orbits about the core of theMilky Way galaxy. Thus, their relative positions change over time, and for the nearer stars this movement can be measured. As astar moves toward or away from us, itsapparent brightness changes.Sirius is currently the brightest star in Earth's night sky, but it has not always been so.Canopus has persistently been the brightest star over the ages; other stars appear brighter only during relatively temporary periods, during which they are passing the Solar System at a much closer distance thanCanopus.

Working out exactly which stars were or will be the brightest at any given point in the past or future is difficult since it requires precise 3D proper motions of large numbers of stars and precise distances, as well as stellar evolution (for massive stars).[1] This information only started to become available with the 1997Hipparcos satellite data release.[1] Jocelyn Tomkin used this data to compile a list of brightest stars in Earth's night sky at each period within the last or next 5 million years.[1] Re-analysis of the Hipparcos data and new data from theGaia spacecraft reveal omissions and revisions necessary in the list. For example, it omitsGliese 710 which in about 1.35 million years is expected to be close enough to have a magnitude of −2.7,[2] as confirmed by theGaia spacecraft.[3][4]

StarStart
year
End
year
Maximum
year
Maximum
magnitude
Distance at
maximum
magnitude (ly)
Current
distance
Current
magnitude
Epsilon Canis Majoris[a]...−4,460,000−4,700,000−3.99344301.50
Beta Canis Majoris[b]−4,460,000−3,700,000−4,420,000−3.65375001.99
Canopus (first time)−3,700,000−1,370,000−3,110,000−1.86177310−0.72
Zeta Leporis−1,080,000−950,000−1,050,000−2.055.3703.55
Canopus (second time)−950,000−420,000−950,000−1.09[c]252310−0.72
Aldebaran−420,000−210,000−320,000−1.5421.5650.85
Capella−210,000−160,000−240,000−0.82[d]27.942.20.08
Canopus (third time)−160,000−90,000−160,000−0.70[c]302310−0.72
Sirius (current)−90,000+210,000+60,000−1.687.88.6−1.46
Vega+210,000+480,000+290,000−0.8117.225.040.03
Canopus (fourth time)+480,000+990,000+480,000−0.40[c]346310−0.72
Beta Aurigae+990,000+1,150,000+1,190,000−0.40[d]28.582.11.9
Delta Scuti+1,150,000+1,260,000+1,250,000−1.849.21874.72
Gliese 710+1,260,000+1,460,000+1,300,000−2.70.16629.66
Gamma Draconis+1,460,000+2,030,000+1,550,000−1.3927.71542.36
Upsilon Librae+2,030,000+2,670,000+2,290,000−0.46301953.6
NR Canis Majoris+2,670,000+3,050,000+2,870,000−0.88142805.6
Omicron Herculis+3,050,000+3,870,000+3,470,000−0.63443463.83
Albireo+3,870,000...+4,610,000−0.52803903.18

Notes

[edit]
  1. ^This star is now a luminous giant. It may have been on the main sequence, approx. 1 mag fainter, during the time span given.
  2. ^This star is now a giant. It may have been on the main sequence, approx. 1 mag fainter, during the time span given.
  3. ^abcPeak magnitude is not the brightest for this star
  4. ^abThis peak occurs when another star is brightest

References

[edit]
  1. ^abcTomkin, Jocelyn (April 1998). "Once and Future Celestial Kings".Sky and Telescope.95 (4):59–63.Bibcode:1998S&T....95d..59T. – based on computations fromHIPPARCOS data. (The calculations exclude stars whose distance orproper motion is uncertain.)PDF[dead link]
  2. ^Berski, Filip; Dybczyński, Piotr A. (2016-11-01)."Gliese 710 will pass the Sun even closer".Astronomy & Astrophysics.595: L10.Bibcode:2016A&A...595L..10B.doi:10.1051/0004-6361/201629835.ISSN 0004-6361.
  3. ^de la Fuente Marcos, Raúl; de la Fuente Marcos, Carlos (10 May 2018)."An Independent Confirmation of the Future Flyby of Gliese 710 to the Solar System UsingGaia".Research Notes of the AAS.2 (2): 30.arXiv:1805.02644.Bibcode:2018RNAAS...2...30D.doi:10.3847/2515-5172/aac2d0.S2CID 119467738.
  4. ^de la Fuente Marcos, Raúl; de la Fuente Marcos, Carlos (10 December 2020)."An Update on the Future Flyby of Gliese 710 to the Solar System Using Gaia EDR3: Slightly Closer and a Tad Later than Previous Estimates".Research Notes of the AAS.4 (12): 222.Bibcode:2020RNAAS...4..222D.doi:10.3847/2515-5172/abd18d.
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