Gliese 710
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Serpens |
| Right ascension | 18h 19m 51s |
| Declination | −01° 56.4′ |
| Apparent magnitude (V) | 9.65–9.69(var) |
| Characteristics | |
| Spectral type | K7V |
| U−B color index | 1.23 |
| B−V color index | 1.36 |
| Variable type | Suspected |
| Astrometry | |
| Radial velocity (Rv) | −24.0 km/s |
| Proper motion (μ) | RA: −130 mas/yr Dec.: −50 mas/yr |
| Parallax (π) | 51.8 ± 7.1 mas |
| Distance | approx. 63 ly (approx. 19 pc) |
| Absolute magnitude (MV) | 8.7 ± 0.3 |
| Details | |
| Mass | 0.6[1] M☉ |
| Radius | 0.67[2] R☉ |
| Luminosity | (bolometric)0.042 L☉ |
| Temperature | 4250[1] K |
| Metallicity | ? |
| Rotation | >14 km/s. |
| Age | ? years |
| Other designations | |
Gliese 710, BD-01 3474, Gl 710, HIP 89825, HD 168442, U449, Vys/McC 63, NSV 10635 | |
Gliese 710 is an orange dwarf star (K7 spectral class) in the constellation Serpens Cauda, with visual magnitude 9.66 and a mass of 0.4–0.6 solar masses.
It is currently about 63.0 light years from Earth, but its proper motion, distance, and radial velocity[3] indicate that it will approach within 1.1 light years (70,000 AU) from Earth within 1.4 million years, based on the latest Hipparcos data. At closest approach it will be a first-magnitude star about as bright as Antares. The proper motion of this star is very small for its distance, meaning it is traveling nearly directly in our line of sight; compare for example with Arcturus.
In a time interval of ±10 million years from the present, Gliese 710 is the star whose combination of mass and close approach distance will cause the greatest gravitational perturbation of our solar system. Specifically, it has the potential to perturb the Oort cloud enough to send a shower of comets into the inner solar system, possibly causing an impact event. However, recent dynamic models by García-Sánchez, et al. indicate that the net increase in cratering rate due to the passage of Gliese 710 will be no more than 5%. They estimate that the closest approach will happen in 1,360,000 years when the star will approach within 0.337 ± 0.177 pc (1.1 ly) of the Sun.[4]
The star with the second greatest perturbational effect in the past or future 10 million years was Algol,[1] a triple star system that passed no closer than 9.8 light years, 7.3 million years ago, but with a considerably larger total mass of 5.8 solar masses. Algol (also known as the Demon Star) was traditionally considered the unluckiest star in the sky, which is reflected in its name (Al-ghol means 'the ghoul' in Arabic)
References
- ^ a b c García-Sánchez, Joan (1999). "Stellar Encounters with the Oort Cloud Based on HIPPARCOS Data". The Astronomical Journal. 117 (2): 1042–1055. Bibcode:1999AJ....117.1042G. doi:10.1086/300723.
{{cite journal}}: Unknown parameter|coauthors=ignored (|author=suggested) (help); Unknown parameter|month=ignored (help) - ^ Johnson H. M. (1983). "Predicted infrared brightness of stars within 25 parsecs of the sun". The Astrophysical Journal Supplement Series. 53: 643–711. Bibcode:1983ApJS...53..643J. doi:10.1086/190905.
{{cite journal}}: Unknown parameter|coauthors=ignored (|author=suggested) (help); Unknown parameter|month=ignored (help) - ^ See also: Stellar kinematics.
- ^ García-Sánchez, J. (2001). "Stellar encounters with the solar system". Astronomy and Astrophysics. 379: 634–659. doi:10.1051/0004-6361:20011330. Retrieved 2008-06-12.
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Further reading
- García-Sánchez, Joan (1999). "Stellar encounters with the Oort cloud based on Hipparcos data". The Astronomical Journal. 117: 1042–1055. doi:10.1086/300723.
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- Searching for Stars Closely Encountering with the Solar System Vadim V. Bobylev - DOI:10.1134/S1063773710030060 - Astronomy Letters, 2010 Vol. 36, No. 3, arXiv:1003.2160v1