HD 110082 b

From Wikipedia
https://en.wikipedia.org/wiki/HD_110082_b
HD 110082 b
Discovery
Discovery dateFebruary 2021
Orbital characteristics
0.113 AU [1]
Eccentricity0.2 [1]
10.18 days [1]
Physical characteristics
Mean radius
3.2  R [1]
Mass11 M [1]

HD 110082 b is a sub-Neptune exoplanet that is three times larger than Earth, orbiting the star HD 110082. The exoplanet's discovery was reported in February 2021. [1]

Further reading

  • Benjamin M. Tofflemire, Aaron C. Rizzuto, Elisabeth R. Newton, Adam L. Kraus, Andrew W. Mann, Andrew Vanderburg, Tyler Nelson, Keith Hawkins, Mackenna L. Wood, George Zhou, Samuel N. Quinn, Steve B. Howell, Karen A. Collins, Richard P. Schwarz, Keivan G. Stassun, Luke G. Bouma, Zahra Essack, Hugh Osborn, Patricia T. Boyd, Gabor Furesz, Ana Glidden, Joseph D. Twicken, Bill Wohler, Brian McLean, George R. Ricker, Roland Vanderspek, David W. Latham, S. Seager, Joshua N. Winn, Jon M. Jenkins: “TESS Hunt for Young and Maturing Exoplanets (THYME) V: A Sub-Neptune Transiting a Young Star in a Newly Discovered 250 Myr Association”, 2021; arXiv:2102.06066.

References

  1. ^ a b c d e f Nowakowski, Tomasz (17 February 2021). "THYME project discovers a sub-Neptune exoplanet orbiting young star". Phys.org. Retrieved 17 February 2021. CS1 maint: discouraged parameter ( link)