HD 48265 b
HD 48265 b is a cold gas giant orbiting HD 48265 in the constellation Puppis. It lies about 295 light-years from Earth and was discovered in 2008 using the radial velocity method. It orbits within the habitable zone of its star — the region where liquid water could exist on a planet's surface.
Is HD 48265 b in the Habitable Zone?
HD 48265 b orbits inside the conservative habitable zone of HD 48265 — the region where a rocky planet could sustain liquid water on its surface. This makes it one of the most interesting known exoplanets in the search for life.
Habitable zone of HD 48265: 1.408–3.322 AU (conservative: 1.784–3.149 AU), per Kopparapu et al. (2014). Earth orbits the Sun at 1 AU.
See the full interactive habitable-zone view in the Exoplanet Explorer app ›
Orbit and Year Length
A year on HD 48265 b — one full orbit around HD 48265 — lasts 778.5 Earth days, longer than an Earth year. It orbits at an average distance of 1.814 AU. Its orbit is mildly elliptical (eccentricity 0.21).
How Was HD 48265 b Discovered?
HD 48265 b was discovered in 2008 using the radial velocity method, with observations from Las Campanas Observatory.
The radial velocity method measures the subtle wobble of a star caused by the gravitational pull of an orbiting planet, visible as periodic shifts in the star's light spectrum. The size of the wobble reveals the planet's minimum mass.
How Far Away Is HD 48265 b?
HD 48265 b is 295.3 light-years (90.5 parsecs) from Earth. Light arriving here tonight left the planet around the year 1731. A probe traveling at the speed of Voyager 1 — about 17 km/s, the fastest outbound spacecraft ever launched — would need roughly 5,197,280 years to make the journey.
Earth Similarity Index
The Earth Similarity Index (ESI) scores how physically similar a planet is to Earth, from 0 to 1, based on radius, density, escape velocity and surface temperature. HD 48265 b scores 0.39, ranking #539 of 5,568 planets with a known ESI. For reference, Mars scores about 0.70.
The Host Star: HD 48265
HD 48265
- Surface temperature
- 5,733 K (Sun: 5,772 K)
- Mass
- 1.31 M☉
- Radius
- 1.90 R☉
- Age
- 4.2 billion years (Sun: 4.6)
The HD 48265 Planetary System
HD 48265 b is one of 2 known planets in the HD 48265 system. Its siblings:
- HD 48265 c (Cold Gas Giant)
HD 48265 b — Complete Data
| Mass (best estimate) | 484.69 Earth masses |
|---|---|
| Orbital period | 778.51 days |
| Orbital distance | 1.814 AU |
| Eccentricity | 0.211 |
| Earth Similarity Index | 0.39 |
| Distance from Earth | 295.3 light-years (90.5 parsecs) |
| Constellation | Puppis |
| Discovery method | Radial Velocity |
| Discovery facility | Las Campanas Observatory |
| Discovery year | 2008 |
Data: NASA Exoplanet Archive, last updated 2019-06-24. Earth Similarity Index: PHL @ UPR Arecibo.
Frequently Asked Questions About HD 48265 b
Is HD 48265 b habitable?
HD 48265 b orbits within the habitable zone of HD 48265, the region where liquid water could exist on a planet's surface. It sits in the conservative habitable zone — the most promising region for habitability. Whether it is actually habitable depends on its atmosphere and composition, which remain unknown.
How far away is HD 48265 b?
HD 48265 b is about 295 light-years from Earth in the constellation Puppis. A spacecraft traveling as fast as Voyager 1 (about 17 km/s) would need roughly 5,197,280 years to get there.
How long is a year on HD 48265 b?
One orbit around HD 48265 takes 778.5 Earth days.
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