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HD 184010
Subgiant star in the constellation Vulpecula From Wikipedia, the free encyclopedia
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HD 184010 is a single evolved star in the constellation of Vulpecula. Its surface temperature is 4,987±10 K. HD 184010 has an orange/red hue and is visible to the naked eye with an apparent visual magnitude of 5.89. Based upon parallax measurements, it is located 200 light-years in distance from the Sun. The object is drifting further away from the Sun with a radial velocity of +5.73±0.12 km/s.[2]
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Planetary system
In 2022, three planets orbiting HD 184010 were discovered by the radial velocity method.[3][4]
None of these three planets orbit in the habitable zone and all are believed to be gas giants.[3]
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See also
Notes
References
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