HD 110067
Appearance
This article or section is in a state of significant expansion or restructuring. You are welcome to assist in its construction by editing it as well. If this article or section has not been edited in several days, please remove this template. If you are the editor who added this template and you are actively editing, please be sure to replace this template with {{in use}} during the active editing session. Click on the link for template parameters to use.
This article was last edited by Madcoverboy (talk | contribs) 11 months ago. (Update timer) |
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | |
Right ascension | 12h 39m 22.0s |
Declination | +20° 18′ 40″ |
Apparent magnitude (V) | 8.4 |
Database references | |
Exoplanet Archive | 110067 data |
HD 110067 is a star with six known sub-Neptune exoplanets with radii ranging from 1.94R⊕ to 2.85R⊕.[1][2][3]
See also
- HD 10180, a star with at least six known planets, and three more exoplanet candidates
- Tabby's Star, another star with notable transit data
- LHS 1140, another star with a planetary system suitable for atmospheric studies
- LP 890-9, the second-coolest star found to host a planetary system, after TRAPPIST-1.
- List of potentially habitable exoplanets
References
- ^ Lugue, R.; et al. (29 November 2023). "A resonant sextuplet of sub-Neptunes transiting the bright star HD 110067". Nature. 623: 932–937. doi:10.1038/s41586-023-06692-3. Archived from the original on 29 November 2023. Retrieved 29 November 2023.
- ^ Clery, Daniel (19 November 2023). "Astronomers stunned by six-planet system frozen in time - Undisturbed family of "sub-Neptunes" in rhythmic orbits could hold clues to planet formation". Science. doi:10.1126/science.ze93fui. Archived from the original on 19 November 2023. Retrieved 19 November 2023.
- ^ Ghosh, Pallab (29 November 2023). "'Perfect solar system' found in search for alien life". BBC. Archived from the original on 29 November 2023. Retrieved 29 November 2023.
Further reading
- The nature and origins of sub-Neptune size planets, Jacob L. Bean, Sean N. Raymond, James E. Owen, 22 Oct 2020