Astronomy:HD 24480

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Short description: Multiple star systemin the constellation Camelopardalis
HD 24480
Observation data
Equinox J2000.0]] (ICRS)
Constellation Camelopardalis[1]
Right ascension  03h 57m 08.2886s[2]
Declination +61° 06′ 31.995″[2]
Apparent magnitude (V) 5.05[3]
Characteristics
Spectral type K4III[4]
U−B color index +1.18[5]
B−V color index +1.42[5]
Astrometry
Radial velocity (Rv)−4.20±0.20[2] km/s
Proper motion (μ) RA: −2.117(96)[2] mas/yr
Dec.: −12.858(99)[2] mas/yr
Parallax (π)3.1699 ± 0.1037[2] mas
Distance1,030 ± 30 ly
(320 ± 10 pc)
Details
Mass1.8[6] M☉
Radius87[7] R☉
Luminosity2,170[7] L☉
Surface gravity (log g)1.75[6] cgs
Temperature4,205[6] K
Metallicity [Fe/H]−0.02[6] dex
Other designations
BD+60°768, HD 24480, HIP 18488A, HR 1205, SAO 12968[8]
Database references
SIMBADdata

HD 24480 is a cool giant star in the northern constellation of Camelopardalis. It has a stellar classification of K4III and an apparent magnitude of 5.05.

The nearby HD 24481 is at a similar distance and shares a common proper motion. It is a hotter, A-[4] or B-type star and a suspected spectroscopic binary system.[9] It is 1.71 arcseconds away from HD 24480.[10]

References

  1. ↑ Roman, Nancy G. (1987). "Identification of a constellation from a position". Publications of the Astronomical Society of the Pacific 99 (617): 695. doi:10.1086/132034. Bibcode: 1987PASP...99..695R  Constellation record for this object at VizieR.
  2. ↑ 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. ↑ Fabricius, C.; Høg, E.; Makarov, V. V.; Mason, B. D.; Wycoff, G. L.; Urban, S. E. (2002). "The Tycho double star catalogue". Astronomy and Astrophysics 384: 180. doi:10.1051/0004-6361:20011822. Bibcode: 2002A&A...384..180F. 
  4. ↑ 4.0 4.1 Abt, Helmut A. (2008). "Visual Multiples. IX. MK Spectral Types". The Astrophysical Journal Supplement Series 176 (1): 216–217. doi:10.1086/525529. Bibcode: 2008ApJS..176..216A. 
  5. ↑ 5.0 5.1 Mermilliod, J.-C. (1986). "Compilation of Eggen's UBV data, transformed to UBV (unpublished)". Catalogue of Eggen's UBV Data. SIMBAD. Bibcode: 1986EgUBV........0M. 
  6. ↑ 6.0 6.1 6.2 6.3 Khalatyan, A.; Anders, F.; Chiappini, C.; Queiroz, A. B. A.; Nepal, S.; Dal Ponte, M.; Jordi, C.; Guiglion, G. et al. (2024). "Transferring spectroscopic stellar labels to 217 million Gaia DR3 XP stars with SHBoost". Astronomy and Astrophysics 691: A98. doi:10.1051/0004-6361/202451427. Bibcode: 2024A&A...691A..98K. 
  7. ↑ 7.0 7.1 Fetherolf, Tara; Pepper, Joshua; Simpson, Emilie; Kane, Stephen R.; Močnik, Teo; English, John Edward; Antoci, Victoria; Huber, Daniel et al. (2023). "Variability Catalog of Stars Observed during the TESS Prime Mission". The Astrophysical Journal Supplement Series 268 (1): 4. doi:10.3847/1538-4365/acdee5. Bibcode: 2023ApJS..268....4F. 
  8. ↑ "HD 24480". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=HD+24480. 
  9. ↑ Parsons, Sidney B. (May 2004). "New and Confirmed Triple Systems with Luminous Cool Primaries and Hot Companions". The Astronomical Journal 127 (5): 2915–2930. doi:10.1086/383546. Bibcode: 2004AJ....127.2915P. 
  10. ↑ Eggleton, P. P.; Tokovinin, A. A. (September 2008). "A catalogue of multiplicity among bright stellar systems". Monthly Notices of the Royal Astronomical Society 389 (2): 869–879. doi:10.1111/j.1365-2966.2008.13596.x. Bibcode: 2008MNRAS.389..869E.