Astronomy:HD 33875
Observation data Equinox J2000.0]] (ICRS) | |
---|---|
Constellation | Mensa |
Right ascension | 05h 06m 09.2953s[1] |
Declination | −73° 02′ 15.6159″[1] |
Apparent magnitude (V) | 6.26 ± 0.01[2] |
Characteristics | |
Spectral type | A1 V[3] or A0 V[4] |
U−B color index | −0.01[5] |
B−V color index | +0.01[5] |
Astrometry | |
Radial velocity (Rv) | 8 ± 7.4[6] km/s |
Proper motion (μ) | RA: +17.783[1] mas/yr Dec.: +63.090[1] mas/yr |
Parallax (π) | 7.742 ± 0.0276[1] mas |
Distance | 421 ± 2 ly (129.2 ± 0.5 pc) |
Absolute magnitude (MV) | +0.7 |
Details | |
Mass | 2.31 ± 0.41[7] M☉ |
Radius | 2.84 ± 0.35[7] R☉ |
Luminosity | 49.2[8] L☉ |
Surface gravity (log g) | 4[9] cgs |
Temperature | 9,392[10] K |
Rotational velocity (v sin i) | 124 ± 6[10] km/s |
Age | 411[11] Myr |
Other designations | |
Database references | |
SIMBAD | data |
HD 33875 (HR 1700) is a solitary star in the southern circumpolar constellation Mensa. With an apparent magnitude of 6.26,[2] it is barely visible to the naked eye under ideal conditions. The star is located at a distance of 421[1] light years but is receding at a rate of 8 km/s.[6]
HD 33875 is an ordinary A-type main-sequence star with a stellar classification of either A1 V[3] or A0 V[4] depending on the source. At present it has 2.38 times the mass of the Sun[7] and 2.84 times the radius of the Sun.[7] It shines at 49.2 times the Sun's luminosity[8] from its photosphere at an effective temperature of 9,392 K,[10] which gives it a white glow. HD 33875 is a fast rotator, spinning rapidly with a projected rotational velocity of 124 km/s.[10]
References
- ↑ 1.0 1.1 1.2 1.3 1.4 1.5 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.
- ↑ 2.0 2.1 Høg, E.; Fabricius, C.; Makarov, V. V.; Urban, S.; Corbin, T.; Wycoff, G.; Bastian, U.; Schwekendiek, P. et al. (March 2000). "The Tycho-2 catalogue of the 2.5 million brightest stars". Astronomy and Astrophysics 355: L27–L30. ISSN 0004-6361. Bibcode: 2000A&A...355L..27H.
- ↑ 3.0 3.1 Houk, N.; Cowley, A. P. (1975). University of Michigan Catalogue of two-dimensional spectral types for the HD stars. Volume I. Declinations -90_ to -53_ƒ0.. Bibcode: 1975mcts.book.....H.
- ↑ 4.0 4.1 Buscombe, W. (1 May 1969). "Line Strengths for Southern OB stars--II: Observations with Moderate Dispersion". Monthly Notices of the Royal Astronomical Society 144 (1): 31–39. doi:10.1093/mnras/144.1.31. ISSN 0035-8711. Bibcode: 1969MNRAS.144...31B.
- ↑ 5.0 5.1 Johnson, H. L.; Mitchell, R. I.; Iriarte, B.; Wisniewski, W. Z. (1966). "UBVRIJKL Photometry of the Bright Stars". Communications of the Lunar and Planetary Laboratory 4: 99–110. Bibcode: 1966CoLPL...4...99J.
- ↑ 6.0 6.1 Kharchenko, N.V.; Scholz, R.-D.; Piskunov, A.E.; Röser, S.; Schilbach, E. (November 2007). "Astrophysical supplements to the ASCC-2.5: Ia. Radial velocities of ~55000 stars and mean radial velocities of 516 Galactic open clusters and associations". Astronomische Nachrichten 328 (9): 889–896. doi:10.1002/asna.200710776. ISSN 0004-6337. Bibcode: 2007AN....328..889K.
- ↑ 7.0 7.1 7.2 7.3 Stassun, Keivan G. et al. (September 2018). "The TESS Input Catalog and Candidate Target List". The Astronomical Journal 156 (3): 102. doi:10.3847/1538-3881/aad050. ISSN 0004-6256. Bibcode: 2018AJ....156..102S.
- ↑ 8.0 8.1 McDonald, I.; Zijlstra, A. A.; Boyer, M. L. (21 November 2012). "Fundamental parameters and infrared excesses of Hipparcos stars: Parameters and IR excesses from Hipparcos". Monthly Notices of the Royal Astronomical Society 427 (1): 343–357. doi:10.1111/j.1365-2966.2012.21873.x. ISSN 0035-8711. Bibcode: 2012MNRAS.427..343M.
- ↑ Kordopatis, G. et al. (17 October 2013). "The Radial Velocity Experiment (Rave): Fourth Data Release". The Astronomical Journal 146 (5): 134. doi:10.1088/0004-6256/146/5/134. ISSN 0004-6256. Bibcode: 2013AJ....146..134K.
- ↑ 10.0 10.1 10.2 10.3 Ammler-von Eiff, M.; Reiners, A. (June 2012). "New measurements of rotation and differential rotation in A-F stars: are there two populations of differentially rotating stars?". Astronomy & Astrophysics 542: A116. doi:10.1051/0004-6361/201118724. ISSN 0004-6361. Bibcode: 2012A&A...542A.116A.
- ↑ "Digital Demo Room - Stellar Structure and Evolution Simulator". http://rainman.astro.illinois.edu/ddr/stellar/intermediate.html.
Original source: https://en.wikipedia.org/wiki/HD 33875.
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