HD 92788 b
HD 92788 b is a cold gas giant orbiting the G6 V star HD 92788 in the constellation Sextans. It lies about 113 light-years from Earth and was discovered in 2000 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 92788 b in the Habitable Zone?
HD 92788 b orbits within the optimistic habitable zone of HD 92788 — the broader region where liquid water might be possible under favorable atmospheric conditions.
Habitable zone of HD 92788: 0.847–1.998 AU (conservative: 1.073–1.894 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 92788 b — one full orbit around HD 92788 — lasts 325.8 Earth days, between the years of Mercury (88 days) and Earth (365 days). It orbits at an average distance of 0.970 AU — comparable to the inner Solar System. Its orbit is highly elliptical (eccentricity 0.35), swinging dramatically closer to and farther from its star.
How Was HD 92788 b Discovered?
HD 92788 b was discovered in 2000 using the radial velocity method, with observations from Multiple Observatories.
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 92788 b?
HD 92788 b is 113.0 light-years (34.7 parsecs) from Earth. Light arriving here tonight left the planet around the year 1913. A probe traveling at the speed of Voyager 1 — about 17 km/s, the fastest outbound spacecraft ever launched — would need roughly 1,988,800 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 92788 b scores 0.39, ranking #519 of 5,568 planets with a known ESI. For reference, Mars scores about 0.70.
The Host Star: HD 92788
HD 92788
- Spectral type
- G6 V
- Surface temperature
- 5,744 K (Sun: 5,772 K)
- Mass
- 1.15 M☉
- Radius
- 1.14 R☉
- Age
- 2.6 billion years (Sun: 4.6)
The HD 92788 Planetary System
HD 92788 b is one of 2 known planets in the HD 92788 system. Its siblings:
- HD 92788 c (Cold Gas Giant)
HD 92788 b — Complete Data
| Mass (best estimate) | 1,195.04 Earth masses |
|---|---|
| Orbital period | 325.80 days |
| Orbital distance | 0.970 AU |
| Eccentricity | 0.350 |
| Earth Similarity Index | 0.39 |
| Distance from Earth | 113.0 light-years (34.7 parsecs) |
| Constellation | Sextans |
| Discovery method | Radial Velocity |
| Discovery facility | Multiple Observatories |
| Discovery year | 2000 |
Data: NASA Exoplanet Archive, last updated 2019-04-08. Earth Similarity Index: PHL @ UPR Arecibo.
Frequently Asked Questions About HD 92788 b
Is HD 92788 b habitable?
HD 92788 b orbits within the habitable zone of HD 92788, the region where liquid water could exist on a planet's surface. Whether it is actually habitable depends on its atmosphere and composition, which remain unknown.
How far away is HD 92788 b?
HD 92788 b is about 113 light-years from Earth in the constellation Sextans. A spacecraft traveling as fast as Voyager 1 (about 17 km/s) would need roughly 1,988,800 years to get there.
How long is a year on HD 92788 b?
One orbit around HD 92788 takes 325.8 Earth days.
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