HD 100307
Appearance
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Hydra |
Right ascension | 11h 32m 23.28291s[1] |
Declination | −26° 44′ 48.4974″[1] |
Apparent magnitude (V) | 6.16[2] |
Characteristics | |
Spectral type | M2 III[3] |
U−B color index | +1.99[4] |
B−V color index | +1.67[4] |
Variable type | Suspected |
Astrometry | |
Radial velocity (Rv) | 34.50 ± 0.6[5] km/s |
Proper motion (μ) | RA: −83.52[1] mas/yr Dec.: 19.85[1] mas/yr |
Parallax (π) | 4.54 ± 0.36 mas[1] |
Distance | 720 ± 60 ly (220 ± 20 pc) |
Details[6] | |
Radius | 67.564 R☉ |
Luminosity | 687.324 ± 72.169 L☉ |
Temperature | 3598 ± 125 K |
Other designations | |
Database references | |
SIMBAD | data |
HD 100307 is a suspected variable star in the constellation of Hydra. Its apparent magnitude is 6.16,[2] but interstellar dust makes it appear 0.346 magnitudes dimmer than it should be.[6] It is located some 340 light-years (104 parecs) away, based on parallax.[1]
HD 100307 is a M-type red giant. It has evolved from the main sequence to a radius of 67.6 times that of the Sun. It emits 687 times as much energy as the Sun at a surface temperature of 3,598 K.[6]
References
- ^ a b c d e f van Leeuwen, F.; et al. (2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics. 474 (2): 653–664. arXiv:0708.1752. Bibcode:2007A&A...474..653V. doi:10.1051/0004-6361:20078357.
- ^ a b Ducati, J. R. (2002). "VizieR Online Data Catalog: Catalogue of Stellar Photometry in Johnson's 11-color system". CDS/ADC Collection of Electronic Catalogues. 2237. Bibcode:2002yCat.2237....0D.
- ^ Houk, Nancy (1982). "Michigan catalogue of two-dimensional spectral types for the HD stars". 3. Ann Arbor, Michigan: Dept. of Astronomy, University of Michigan. Bibcode:1982mcts.book.....H.
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(help) - ^ a b Mermilliod, J.-C. (1986). "Compilation of Eggen's UBV data, transformed to UBV (unpublished)". Bibcode:1986EgUBV........0M.
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(help) - ^ Gontcharov, G. A. (2006). "Pulkovo Compilation of Radial Velocities for 35 495 Hipparcos stars in a common system". Astronomy Letters. 32 (11): 759–771. arXiv:1606.08053. Bibcode:2006AstL...32..759G. doi:10.1134/S1063773706110065.
- ^ a b c 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: 770. arXiv:1706.02208. Bibcode:2017MNRAS.471..770M. doi:10.1093/mnras/stx1433.
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