HD 96167 b
HD 96167 b is a cold gas giant orbiting HD 96167 in the constellation Crater. It lies about 278 light-years from Earth and was discovered in 2009 using the radial velocity method.
Is HD 96167 b in the Habitable Zone?
HD 96167 b orbits inside the inner edge of the habitable zone of HD 96167. So close to its star, surface conditions are far too hot for liquid water.
Habitable zone of HD 96167: 1.437–3.390 AU (conservative: 1.820–3.214 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 96167 b — one full orbit around HD 96167 — lasts 498.0 Earth days, longer than an Earth year. It orbits at an average distance of 1.332 AU. Its orbit is highly elliptical (eccentricity 0.69), swinging dramatically closer to and farther from its star.
How Was HD 96167 b Discovered?
HD 96167 b was discovered in 2009 using the radial velocity method, with observations from W. M. Keck 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 96167 b?
HD 96167 b is 278.2 light-years (85.3 parsecs) from Earth. Light arriving here tonight left the planet around the year 1748. A probe traveling at the speed of Voyager 1 — about 17 km/s, the fastest outbound spacecraft ever launched — would need roughly 4,896,320 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 96167 b scores 0.30, ranking #1,433 of 5,568 planets with a known ESI. For reference, Mars scores about 0.70.
The Host Star: HD 96167
HD 96167 b belongs to a system of 2 stars; it orbits HD 96167.
HD 96167
- Surface temperature
- 5,733 K (Sun: 5,772 K)
- Mass
- 1.27 M☉
- Radius
- 1.94 R☉
Planetary System
HD 96167 b is the only planet known to orbit HD 96167 so far.
HD 96167 b — Complete Data
| Mass (best estimate) | 227.88 Earth masses |
|---|---|
| Orbital period | 498.04 days |
| Orbital distance | 1.332 AU |
| Eccentricity | 0.685 |
| Earth Similarity Index | 0.30 |
| Distance from Earth | 278.2 light-years (85.3 parsecs) |
| Constellation | Crater |
| Discovery method | Radial Velocity |
| Discovery facility | W. M. Keck Observatory |
| Discovery year | 2009 |
Data: NASA Exoplanet Archive, last updated 2018-12-03. Earth Similarity Index: PHL @ UPR Arecibo.
Frequently Asked Questions About HD 96167 b
Is HD 96167 b habitable?
No — HD 96167 b orbits too close to its star and is too hot for liquid water to exist on its surface.
How far away is HD 96167 b?
HD 96167 b is about 278 light-years from Earth in the constellation Crater. A spacecraft traveling as fast as Voyager 1 (about 17 km/s) would need roughly 4,896,320 years to get there.
How long is a year on HD 96167 b?
One orbit around HD 96167 takes 498.0 Earth days.