HIP 19976 b
131.35 light-years
Radial Velocity · 2022
System: HIP 19976 →Beyond the Sun
Exoplanets
Confirmed planets from the NASA Exoplanet Archive. Explore a system, or locate its host on the galaxy map.
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HIP 21152 b
141.58 light-years
Imaging · 2022
System: HIP 21152 →HIP 29442 c
222.41 light-years
Radial Velocity · 2023
System: TOI-469 →HIP 29442 d
222.41 light-years
Radial Velocity · 2023
System: TOI-469 →HIP 34222 b
74.49 light-years
Radial Velocity · 2021
System: HIP 34222 →HIP 35173 b
108.14 light-years
Radial Velocity · 2019
System: HIP 35173 →HIP 35965 b
163.63 light-years
Radial Velocity · 2022
System: HIP 35965 →HIP 38594 b
58.02 light-years
Radial Velocity · 2020
System: HIP 38594 →HIP 38594 c
58.02 light-years
Radial Velocity · 2020
System: HIP 38594 →HIP 39017 b
216.31 light-years
Imaging · 2024
System: HIP 39017 →HIP 39330 b
118.71 light-years
Radial Velocity · 2026
System: HIP 39330 →HIP 41378 b
346.67 light-years
Transit · 2016
System: HIP 41378 →HIP 41378 c
346.67 light-years
Transit · 2016
System: HIP 41378 →HIP 41378 d
346.67 light-years
Transit · 2016
System: HIP 41378 →HIP 41378 e
346.67 light-years
Transit · 2016
System: HIP 41378 →HIP 41378 f
346.67 light-years
Transit · 2016
System: HIP 41378 →HIP 41378 g
346.67 light-years
Radial Velocity · 2025
System: HIP 41378 →HIP 4845 b
68.81 light-years
Radial Velocity · 2020
System: HIP 4845 →HIP 48714 b
34.34 light-years
Radial Velocity · 2020
System: HIP 48714 →HIP 5158 b
168.31 light-years
Radial Velocity · 2009
System: HIP 5158 →HIP 5158 c
168.31 light-years
Radial Velocity · 2011
System: HIP 5158 →HIP 54373 b
61.05 light-years
Radial Velocity · 2019
System: HIP 54373 →HIP 54373 c
61.05 light-years
Radial Velocity · 2019
System: HIP 54373 →HIP 54515 b
270.09 light-years
Imaging · 2026
System: HIP 54515 →Download this filtered page
Up to 24 planets with original measurements, uncertainties, limits and references. JSON preserves missing fields and null values; CSV includes the original source data as JSON alongside measurement columns. The catalogue can change between viewing and downloading. When supplied by the backend, exports retain the catalogue identity read with that downloaded page. Older responses remain unassociated, and an unknown identity remains unknown. This does not pin your earlier view or subsequent pages.
Data: NASA Exoplanet Archive, Planetary Systems Composite Parameters (PSCompPars). This is a catalogue of discoveries, not a complete census of planets.