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Red dwarf
30 Arietis Bb (sometimes abbreviated 30 Ari Bb ) is a red dwarf which orbits the F-type main sequence star 30 Arietis Ba , located in a quintuple star system approximately 146 light years away in the constellation Aries . The red dwarf was discovered by on Friday, November 27, 2009 by using precise radial velocity method from echelle spectrograph installed in the Alfred-Jensch telescope in Karl Schwarzschild Observatory . The star had a minimum mass of nearly 10 times that of Jupiter . In 2020, after the inclination of the planetary orbit was measured to be just 4.14−0.90 °, the "planet" was found to fall in the mass range of the red dwarf star.
References
^ Kiefer, Flavien; Hébrard, Guillaume; Lecavelier, Alain; Martioli, Eder; Dalal, Shweta; Vidal-Madjar, Alfred (2021), "Determining the true mass of radial-velocity exoplanets with Gaia 9 planet candidates in the brown-dwarf/stellar regime and 27 confirmed planets", Astronomy & Astrophysics , A7 : 645, arXiv :2009.14164 , doi :10.1051/0004-6361/202039168 , S2CID 221995447
Guenther, E. W.; et al. (2009). "A substellar component orbiting the F-star 30 Arietis B" . Astronomy and Astrophysics . 507 (3): 1659–1665. arXiv :0912.4619 . Bibcode :2009A&A...507.1659G . doi :10.1051/0004-6361/200912112 .
Jean Schneider (2011). "Notes for Planet 30 Ari B b" . Extrasolar Planets Encyclopaedia . Retrieved 3 October 2011.
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