HD 93385 d
HD 93385 d is a super-Earth orbiting the G2/G3 V star HD 93385 in the constellation Vela. It lies about 141 light-years from Earth and was discovered in 2021 using the radial velocity method.
Is HD 93385 d in the Habitable Zone?
HD 93385 d orbits inside the inner edge of the habitable zone of HD 93385. So close to its star, surface conditions are far too hot for liquid water.
Habitable zone of HD 93385: 0.941–2.206 AU (conservative: 1.192–2.091 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 93385 d — one full orbit around HD 93385 — lasts 45.9 Earth days, shorter than Mercury's 88-day year. It orbits at an average distance of 0.257 AU — closer to its star than Mercury is to the Sun. Its orbit is mildly elliptical (eccentricity 0.09).
How Was HD 93385 d Discovered?
HD 93385 d was discovered in 2021 using the radial velocity method, with observations from La Silla 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 93385 d?
HD 93385 d is 141.4 light-years (43.3 parsecs) from Earth. Light arriving here tonight left the planet around the year 1885. A probe traveling at the speed of Voyager 1 — about 17 km/s, the fastest outbound spacecraft ever launched — would need roughly 2,488,640 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 93385 d scores 0.26, ranking #2,788 of 5,568 planets with a known ESI. For reference, Mars scores about 0.70.
The Host Star: HD 93385
HD 93385
- Spectral type
- G2/G3 V
- Surface temperature
- 5,977 K (Sun: 5,772 K)
- Mass
- 1.04 M☉
- Luminosity
- 1.6100 L☉
- Age
- 3.3 billion years (Sun: 4.6)
The HD 93385 Planetary System
HD 93385 d is one of 3 known planets in the HD 93385 system. Its siblings:
- HD 93385 b (Super Earth)
- HD 93385 c (Super Earth)
HD 93385 d — Complete Data
| Mass (best estimate) | 8.70 Earth masses |
|---|---|
| Orbital period | 45.85 days |
| Orbital distance | 0.257 AU |
| Eccentricity | 0.090 |
| Earth Similarity Index | 0.26 |
| Distance from Earth | 141.4 light-years (43.3 parsecs) |
| Constellation | Vela |
| Discovery method | Radial Velocity |
| Discovery facility | La Silla Observatory |
| Discovery year | 2021 |
Data: NASA Exoplanet Archive, last updated 2021-11-04. Earth Similarity Index: PHL @ UPR Arecibo.
Frequently Asked Questions About HD 93385 d
Is HD 93385 d habitable?
No — HD 93385 d orbits too close to its star and is too hot for liquid water to exist on its surface.
How far away is HD 93385 d?
HD 93385 d is about 141 light-years from Earth in the constellation Vela. A spacecraft traveling as fast as Voyager 1 (about 17 km/s) would need roughly 2,488,640 years to get there.
How long is a year on HD 93385 d?
One orbit around HD 93385 takes 45.9 Earth days.
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