Astronomy:Gliese 445

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Short description: Star in the constellation Camelopardalis

Coordinates: Sky map 11h 47m 41.3885s, +78° 41′ 28.179″

Gliese 445
PIA17461 Heading toward Gliese 445 (annotated).jpg
Image of AC +79 3888 (circled), also known as Gliese 445, located 17.1 light-years from Earth
Credit: Caltech/Palomar
Observation data
Equinox J2000.0]] (ICRS)
Constellation Camelopardalis
Right ascension  11h 47m 41.3885s[1]
Declination +78° 41′ 28.179″[1]
Apparent magnitude (V) 10.80[2]
Characteristics
Spectral type M4.0Ve[3]
B−V color index 1.572[2]
Astrometry
Radial velocity (Rv)−111.707[1] km/s
Proper motion (μ) RA: 748.111[1] mas/yr
Dec.: 480.804[1] mas/yr
Parallax (π)190.3251 ± 0.0194[4] mas
Distance17.137 ± 0.002 ly
(5.2542 ± 0.0005 pc)
Absolute magnitude (MV)12.227[5]
Details
Mass0.14[6] M☉
Radius0.285[5] R☉
Luminosity0.008[7] L☉
Surface gravity (log g)4.72[7] cgs
Temperature3,507[1] K
Metallicity [Fe/H]−0.30[5] dex
Rotational velocity (v sin i)<2.5[8] km/s
Other designations
Gliese 445, Gl 445, G 254-29, AC+79 3888, HIP 57544, LFT 849, LHS 2459, LTT 13235, NLTT 28539, PLX 2722[9]
Database references
SIMBADdata
ARICNSdata
Gliese 445 is located in the constellation Camelopardalis
Gliese 445 is located in the constellation Camelopardalis
Gliese 445
Location of Gliese 445 in the constellation Camelopardalis

Gliese 445 (Gl 445 or AC +79 3888) is an M-type main sequence star in the northern part of the constellation Camelopardalis.

Location

Distances of the nearest stars from 20,000 years ago until 80,000 years in the future

It is currently 17.1 light-years from Earth and has an apparent magnitude of 10.8. It is visible from north of the Tropic of Cancer all night long, but not to the naked eye.[10] Because the star is a red dwarf with a mass only a quarter to a third of that of the Sun, scientists question the ability of this system to support life.[10] Gliese 445 is also a known X-ray source.[11]

The Voyager 1 probe will pass within 1.6 light-years of Gliese 445 in about 40,000 years.[12]

Solar encounter

While the Voyager probe moves through space towards a 1.6-light-year minimum distance from Gliese 445, the star is rapidly approaching the Sun. At the time the probe passes Gliese 445, the star will be about 1.059 parsecs (3.45 light-years) from the Sun,[13] but with less than half the brightness necessary to be seen with the naked eye.[10] At that time, Gliese 445 will be approximately tied with Ross 248 for being the closest star to the Sun (see List of nearest stars#Future and past).

See also

References

  1. ↑ 1.0 1.1 1.2 1.3 1.4 1.5 Brown, A. G. A. (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics 616: A1. doi:10.1051/0004-6361/201833051. Bibcode: 2018A&A...616A...1G.  Gaia DR2 record for this source at VizieR.
  2. ↑ 2.0 2.1 Urban, S. E.; Zacharias, N.; Wycoff, Observatory G. L. U. S. Naval; Washington, 2004-2006 D. C. (2004). "VizieR Online Data Catalog: The UCAC2 Bright Star Supplement (Urban+, 2006)". VizieR On-line Data Catalog. Bibcode: 2004yCat.1294....0U. 
  3. ↑ Lépine, Sébastien; Hilton, Eric J.; Mann, Andrew W.; Wilde, Matthew; Rojas-Ayala, Bárbara; Cruz, Kelle L.; Gaidos, Eric (2013). "A Spectroscopic Catalog of the Brightest (J < 9) M Dwarfs in the Northern Sky". The Astronomical Journal 145 (4): 102. doi:10.1088/0004-6256/145/4/102. Bibcode: 2013AJ....145..102L. 
  4. ↑ Brown, A. G. A. (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics 649: A1. doi:10.1051/0004-6361/202039657. Bibcode: 2021A&A...649A...1G.  Gaia EDR3 record for this source at VizieR.
  5. ↑ 5.0 5.1 5.2 Houdebine, Éric R.; Mullan, D. J.; Doyle, J. G.; de la Vieuville, Geoffroy; Butler, C. J.; Paletou, F. (2019). "The Mass-Activity Relationships in M and K Dwarfs. I. Stellar Parameters of Our Sample of M and K Dwarfs". The Astronomical Journal 158 (2): 56. doi:10.3847/1538-3881/ab23fe. Bibcode: 2019AJ....158...56H. 
  6. ↑ Gaidos, E.; Mann, A. W.; Lépine, S.; Buccino, A.; James, D.; Ansdell, M.; Petrucci, R.; Mauas, P. et al. (2014). "Trumpeting M dwarfs with CONCH-SHELL: A catalogue of nearby cool host-stars for habitable exoplanets and life". Monthly Notices of the Royal Astronomical Society 443 (3): 2561. doi:10.1093/mnras/stu1313. Bibcode: 2014MNRAS.443.2561G. 
  7. ↑ 7.0 7.1 McDonald, I.; Zijlstra, A. A.; Watson, R. A. (2017). "Fundamental parameters and infrared excesses of Tycho-Gaia stars". Monthly Notices of the Royal Astronomical Society 471 (1): 770. doi:10.1093/mnras/stx1433. Bibcode: 2017MNRAS.471..770M. 
  8. ↑ Stelzer, B.; Marino, A.; Micela, G.; López-Santiago, J.; Liefke, C. (2013). "The UV and X-ray activity of the M dwarfs within 10 pc of the Sun". Monthly Notices of the Royal Astronomical Society 431 (3): 2063. doi:10.1093/mnras/stt225. Bibcode: 2013MNRAS.431.2063S. 
  9. ↑ "GJ 445". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=GJ+445. 
  10. ↑ 10.0 10.1 10.2 Mark Littmann (1 January 2004). Planets Beyond: Discovering the Outer Solar System. Courier Corporation. ISBN 978-0-486-43602-9. https://books.google.com/books?id=RoJMadct4TQC. 
  11. ↑ Schmitt JHMM; Fleming TA; Giampapa MS (September 1995). "The X-Ray View of the Low-Mass Stars in the Solar Neighborhood". Astrophys. J. 450 (9): 392–400. doi:10.1086/176149. Bibcode: 1995ApJ...450..392S. 
  12. ↑ "NASA – Voyager - Mission - Interstellar Mission". http://voyager.jpl.nasa.gov/mission/interstellar.html. 
  13. ↑ Bobylev, Vadim V. (March 2010). "Searching for Stars Closely Encountering with the Solar System". Astronomy Letters 36 (3): 220–226. doi:10.1134/S1063773710030060. Bibcode: 2010AstL...36..220B. 

External links

  • Wikisky image of TYC 4553-192-1 (Gliese 445)



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