Star in the constellation of Pegasus
35 Pegasi
Location of 35 Pegasi (circled)
Observation dataEpoch J2000 Equinox J2000
Constellation
Pegasus
Right ascension
22 27 51.52233
Declination
4° 41′ 44.3916″
Apparent magnitude (V)
4.80
Characteristics
Evolutionary stage
horizontal branch
Spectral type
K0III
U−B color index
+0.88
B−V color index
+1.06
Astrometry Radial velocity (Rv )+54.16 km/s Proper motion (μ) RA: +77.57 mas /yr Dec.: −306.12 mas /yr Parallax (π)21.0039 ± 0.2419 mas Distance 155 ± 2 ly (47.6 ± 0.5 pc ) Absolute magnitude (MV )1.50
Details Mass 1.18 M ☉ Radius 8.5 R ☉ Luminosity 31.69 L ☉ Surface gravity (log g )2.76 cgs Temperature 4,676 K Metallicity −0.28 dex Rotational velocity (v sin i )1.5 km/s Age 4.94 Gyr
Other designations 35 Peg , BD +03°4710, FK5 3796, GC 31377, HD 212943, HIP 110882, HR 8551, SAO 127540, CCDM J22278+0441A, WDS J22279+0442A, LTT 16582
Database references SIMBAD data
35 Pegasi is a single star in the northern constellation of Pegasus . It is visible to the naked eye as a faint, orange-hued point of light with an apparent visual magnitude of 4.80. The star is located approximately 155 light years away from the Sun based on parallax , and is drifting further away with a radial velocity of +54 km/s. The star has a relatively high proper motion , traversing the celestial sphere at the rate of 0.318 arc seconds per annum.
This is an aging giant star with a stellar classification of K0III, having exhausted the hydrogen at its core and expanded to 8.5 times the Sun's radius . It is a red clump giant, indicating it is on the horizontal branch and is generating energy through helium fusion at its core . The star is five billion years old with 1.2 times the mass of the Sun . It is radiating 32 times the Sun's luminosity from its enlarged photosphere at an effective temperature of 4,676 K.
There are two distant visual companions: component B, at an angular separation of 80.5″ and magnitude 10.0, and C, at separation 176.3″ and magnitude 10.64.
References
^ Brown, A. G. A. ; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties" . Astronomy & Astrophysics . 616 . A1. arXiv :1804.09365 . Bibcode :2018A&A...616A...1G . doi :10.1051/0004-6361/201833051 . Gaia DR2 record for this source at VizieR .
^ 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 .
^ Frasca, A.; et al. (December 2009). "REM near-IR and optical photometric monitoring of pre-main sequence stars in Orion. Rotation periods and starspot parameters". Astronomy and Astrophysics . 508 (3): 1313–1330. arXiv :0911.0760 . Bibcode :2009A&A...508.1313F . doi :10.1051/0004-6361/200913327 . S2CID 118361131 .
^ Famaey, B.; et al. (2005). "Local kinematics of K and M giants from CORAVEL/Hipparcos/Tycho-2 data". Astronomy & Astrophysics . 430 : 165–186. arXiv :astro-ph/0409579 . Bibcode :2005A&A...430..165F . doi :10.1051/0004-6361:20041272 . S2CID 17804304 .
^ Van Leeuwen, F. (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 . S2CID 18759600 . Vizier catalog entry
^ Da Silva, Ronaldo; et al. (2015). "Homogeneous abundance analysis of FGK dwarf, subgiant, and giant stars with and without giant planets". Astronomy & Astrophysics . 580 : A24. arXiv :1505.01726 . Bibcode :2015A&A...580A..24D . doi :10.1051/0004-6361/201525770 . S2CID 119216425 . Vizier catalog entry
^ Allende Prieto, C.; Lambert, D. L. (1999). "Fundamental parameters of nearby stars from the comparison with evolutionary calculations: Masses, radii and effective temperatures". Astronomy and Astrophysics . 352 : 555–562. arXiv :astro-ph/9911002 . Bibcode :1999A&A...352..555A . Vizier catalog entry
^ Anderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation". Astronomy Letters . 38 (5): 331. arXiv :1108.4971 . Bibcode :2012AstL...38..331A . doi :10.1134/S1063773712050015 . S2CID 119257644 . Vizier catalog entry
^ Wu, Yue; et al. (2010). "Coudé-feed stellar spectral library – atmospheric parameters". Astronomy & Astrophysics . 525 : A71. arXiv :1009.1491 . Bibcode :2011A&A...525A..71W . doi :10.1051/0004-6361/201015014 . S2CID 53480665 .
Massarotti, Alessandro; et al. (January 2008). "Rotational and Radial Velocities for a Sample of 761 HIPPARCOS Giants and the Role of Binarity" . The Astronomical Journal . 135 (1): 209–231. Bibcode :2008AJ....135..209M . doi :10.1088/0004-6256/135/1/209 .
^ Luck, R. Earle (2015). "Abundances in the Local Region. I. G and K Giants". Astronomical Journal . 150 (3). 88. arXiv :1507.01466 . Bibcode :2015AJ....150...88L . doi :10.1088/0004-6256/150/3/88 . S2CID 118505114 .
"35 Peg" . SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2019-07-01.
Eggleton, P. P.; Tokovinin, A. A. (2008). "A catalogue of multiplicity among bright stellar systems" . Monthly Notices of the Royal Astronomical Society . 389 (2): 869. arXiv :0806.2878 . Bibcode :2008MNRAS.389..869E . doi :10.1111/j.1365-2966.2008.13596.x . S2CID 14878976 .
Lépine, Sébastien; Shara, Michael M. (March 2005). "A Catalog of Northern Stars with Annual Proper Motions Larger than 0.15" (LSPM-NORTH Catalog)". The Astronomical Journal . 129 (3): 1483–1522. arXiv :astro-ph/0412070 . Bibcode :2005AJ....129.1483L . doi :10.1086/427854 . S2CID 2603568 .
^ Tautvaišienė, G.; et al. (December 2010). "C, N and O abundances in red clump stars of the Milky Way" . Monthly Notices of the Royal Astronomical Society . 409 (3): 1213–1219. arXiv :1007.4064 . Bibcode :2010MNRAS.409.1213T . doi :10.1111/j.1365-2966.2010.17381.x . S2CID 119182458 .
Mason, Brian D.; et al. (2001). "The 2001 US Naval Observatory Double Star CD-ROM. I. The Washington Double Star Catalog" . The Astronomical Journal . 122 (6): 3466. Bibcode :2001AJ....122.3466M . doi :10.1086/323920 . Vizier catalog entry
Categories :
Text is available under the Creative Commons Attribution-ShareAlike License. Additional terms may apply.
**DISCLAIMER** We are not affiliated with Wikipedia, and Cloudflare.
The information presented on this site is for general informational purposes only and does not constitute medical advice.
You should always have a personal consultation with a healthcare professional before making changes to your diet, medication, or exercise routine.
AI helps with the correspondence in our chat.
We participate in an affiliate program. If you buy something through a link, we may earn a commission 💕
↑