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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 |website= |publisher=] |accessdate=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>
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>
==References==
==References==
Revision as of 22:30, 29 December 2020
It has been suggested that this article be merged into 30 Arietis. (Discuss) Proposed since December 2020.
The red dwarf 30 Arietis Bb 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
^ Determining the true mass of radial-velocity exoplanets with Gaia 9 planet candidates in the brown-dwarf/stellar regime and 27 confirmed planets, 2020, arXiv:2009.14164 Cite error: The named reference "Kiefer2020" was defined multiple times with different content (see the help page).
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