Astronomy:LP Aquarii
From HandWiki
Short description: Star in the constellation Aquarius
Observation data Equinox J2000.0]] (ICRS) | |
---|---|
Constellation | Aquarius |
Right ascension | 22h 42m 06.026s[2] |
Declination | −05° 06′ 07.03″[2] |
Apparent magnitude (V) | 6.30 - 6.64[3] |
Characteristics | |
Spectral type | M4III[4] |
Variable type | Lb[5] |
Astrometry | |
Radial velocity (Rv) | −175.81[2] km/s |
Proper motion (μ) | RA: +69.323[2] mas/yr Dec.: −49.636[2] mas/yr |
Parallax (π) | 3.6849 ± 0.1178[2] mas |
Distance | 890 ± 30 ly (271 ± 9 pc) |
Absolute magnitude (MV) | −0.307[6] |
Details | |
Mass | 1.558[7] M☉ |
Radius | 83+15 −11[8] R☉ |
Luminosity | 1,011±66[8] L☉ |
Surface gravity (log g) | 0.476[9] cgs |
Temperature | 3,582+254 −278[8] K |
Metallicity [Fe/H] | −0.045[7] dex |
Other designations | |
Database references | |
SIMBAD | data |
LP Aquarii is a pulsating variable star in the constellation of Aquarius that varies between magnitudes 6.30 and 6.64.[3] The position of the star near the ecliptic means it is subject to lunar occultations.[11]
References
- ↑ "/ftp/cats/more/HIP/cdroms/cats". Strasbourg astronomical Data Center. https://cdsarc.cds.unistra.fr/viz-bin/ftp-index?/ftp/cats/more/HIP/cdroms/cats.
- ↑ 2.0 2.1 2.2 2.3 2.4 Vallenari, A. et al. (2022). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy & Astrophysics. doi:10.1051/0004-6361/202243940 Gaia DR3 record for this source at VizieR.
- ↑ 3.0 3.1 Watson, Christopher (4 January 2010). "LP Aquarii". AAVSO Website. American Association of Variable Star Observers. https://www.aavso.org/vsx/index.php?view=detail.top&oid=1109.
- ↑ Houk, N.; Swift, C. (1999). "Michigan catalogue of two-dimensional spectral types for the HD Stars". Michigan Spectral Survey 5. Bibcode: 1999MSS...C05....0H.
- ↑ Samus, N. N. et al. (2009). "General Catalogue of Variable Stars (Samus+ 2007-2013)". VizieR On-line Data Catalog: B/GCVS. Originally Published in: 2009yCat....102025S 1. Bibcode: 2009yCat....102025S.
- ↑ Gontcharov, G. A. (2011). "The red giant branch in the Tycho-2 catalogue". Astronomy Letters 37 (10): 707–717. doi:10.1134/S1063773711090040. Bibcode: 2011AstL...37..707G.
- ↑ 7.0 7.1 Huber, Daniel; Bryson, Stephen T.; Haas, Michael R.; Barclay, Thomas; Barentsen, Geert; Howell, Steve B.; Sharma, Sanjib; Stello, Dennis et al. (2016). "The K2 Ecliptic Plane Input Catalog (Epic) and Stellar Classifications of 138,600 Targets in Campaigns 1–8". The Astrophysical Journal Supplement Series 224 (1): 2. doi:10.3847/0067-0049/224/1/2. Bibcode: 2016ApJS..224....2H.
- ↑ 8.0 8.1 8.2 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.
- ↑ 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.
- ↑ "LP Aqr". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=LP+Aqr.
- ↑ Morbey, C. L. et al. (December 1978). "Photoelectric Observations of Lunar Occultations at the D.A.O.". Journal of the Royal Astronomical Society of Canada 72: 305. Bibcode: 1978JRASC..72..305M.
Original source: https://en.wikipedia.org/wiki/LP Aquarii.
Read more |