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==Overview== |
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==Overview== |
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The red dwarf 30 Arietis Bb had a ] of nearly 10 times that of ].<ref>{{cite web |url=http://exoplanet.eu/planet.php?p1=30+Ari+B&p2=b |title=Notes for Planet 30 Ari B b |author=Jean Schneider |year=2011 |publisher=] |access-date=3 October 2011}}</ref> In 2020, after the inclination of the planetary orbit was measured to be just 4.14{{±|0.96|0.90}}°, the "planet" was found to fall in the mass range of the red dwarf star.<ref name=Kiefer2020>{{citation|arxiv=2009.14164|title=Determining the true mass of radial-velocity exoplanets with Gaia 9 planet candidates in the brown-dwarf/stellar regime and 27 confirmed planets|year=2020}}</ref> |
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The red dwarf 30 Arietis Bb had a ] of nearly 10 times that of ].<ref>{{cite web |url=http://exoplanet.eu/planet.php?p1=30+Ari+B&p2=b |title=Notes for Planet 30 Ari B b |author=Jean Schneider |year=2011 |publisher=] |access-date=3 October 2011}}</ref> In 2020, after the inclination of the planetary orbit was measured to be just 4.14{{±|0.96|0.90}}°, the "planet" was found to fall in the mass range of the red dwarf star.<ref name=Kiefer2020>{{citation|arxiv=2009.14164|title=Determining the true mass of radial-velocity exoplanets with Gaia 9 planet candidates in the brown-dwarf/stellar regime and 27 confirmed planets|year=2021|doi=10.1051/0004-6361/202039168|last1=Kiefer|first1=Flavien|last2=Hébrard|first2=Guillaume|last3=Lecavelier|first3=Alain|last4=Martioli|first4=Eder|last5=Dalal|first5=Shweta|last6=Vidal-Madjar|first6=Alfred|journal=Astronomy & Astrophysics|volume=A7|page=645|s2cid=221995447}}</ref> |
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==References== |
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==References== |
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