HD 70514

HD 70514 (HR 3280) is a solitary star located in the southern circumpolar constellation Volans. With an apparent magnitude of 5.06, its faintly visible to the naked eye. The star is located 296 light years away from the Solar System, and is drifting away with a radial velocity of 1.98 km/s.

HD 70514

HD 70514 (left) compared to the Sun
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Volans
Right ascension 08h 18m 18.81s[1]
Declination −65° 36 47.49[1]
Apparent magnitude (V) 5.06±0.01[2]
Characteristics
Evolutionary stage RGB[3]
Spectral type K1 III[4]
B−V color index +1.13[5]
Astrometry
Radial velocity (Rv)1.98±0.26[1] km/s
Proper motion (μ) RA: +21.062[1] mas/yr
Dec.: +21.851[1] mas/yr
Parallax (π)11.0219 ± 0.0985 mas[1]
Distance296 ± 3 ly
(90.7 ± 0.8 pc)
Absolute magnitude (MV)+0.26
Details
Mass1.88±0.29[3] M
Radius15.04+0.92
−1.91
[1] R
Luminosity99±1[1] L
Temperature4,515[3] K
Metallicity [Fe/H]+0.1[6] dex
Rotational velocity (v sin i)<1[7] km/s
Other designations
HD 70514 CPD-65 907, HIP 40680, HR 3280
Database references
SIMBADdata

Properties

HD 70514 is classified as a "K1 III" star, which means that this is a giant star that has exhausted hydrogen at its core and left the main sequence. It has 1.9 times the mass of the Sun but has expanded to 15 times the sun's diameter. It radiates at 99 solar luminosities from its enlarged photosphere at an effective temperature of 4,515 K, which gives it an orangish-yellow hue. HD 70514 has a metallicity 126% that of the Sun, and it rotates rather slowly.

References

  1. 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.
  2. Høg, E.; Fabricius, C.; Makarov, V. V.; Urban, S.; Corbin, T.; Wycoff, G.; Bastian, U.; Schwekendiek, P.; Wicenec, A. (March 2000). "The Tycho-2 catalogue of the 2.5 million brightest stars". Astronomy and Astrophysics. 355: L27–L30. Bibcode:2000A&A...355L..27H. ISSN 0004-6361.
  3. Stello, D.; Bruntt, H.; Preston, H.; Buzasi, D. (2008). "Oscillating K Giants with the WIRE Satellite: Determination of Their Asteroseismic Masses". The Astrophysical Journal. 674 (1): L53–L56. arXiv:0801.2155. Bibcode:2008ApJ...674L..53S. doi:10.1086/528936. S2CID 15094067.
  4. Kharchenko, N. V. (October 2001). "All-sky compiled catalogue of 2.5 million stars". Kinematika i Fizika Nebesnykh Tel. 17: 409–423. Bibcode:2001KFNT...17..409K. ISSN 0233-7665.
  5. Allende Prieto, C.; Lambert, D. L. (1999-12-01). "Fundamental parameters of nearby stars from the comparison with evolutionary calculations: masses, radii and effective temperatures". Astronomy and Astrophysics. 352: 555–562. Bibcode:1999A&A...352..555A. ISSN 0004-6361.
  6. Charbonnel, C.; Lagarde, N.; Jasniewicz, G.; North, P. L.; Shetrone, M.; Krugler Hollek, J.; Smith, V. V.; Smiljanic, R.; Palacios, A.; Ottoni, G. (January 2020). "Lithium in red giant stars: Constraining non-standard mixing with large surveys in the Gaia era". Astronomy and Astrophysics. 633: A34. Bibcode:2020A&A...633A..34C. doi:10.1051/0004-6361/201936360. ISSN 0004-6361.
  7. De Medeiros, J. R.; Alves, S.; Udry, S.; Andersen, J.; Nordström, B.; Mayor, M. (2014-01-01). "A catalog of rotational and radial velocities for evolved stars. V. Southern stars". Astronomy and Astrophysics. 561: A126. Bibcode:2014A&A...561A.126D. doi:10.1051/0004-6361/201220762. ISSN 0004-6361.
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