54 Piscium Ab
A Saturn-mass exoplanet with a highly eccentric orbit.
54 Piscium Ab (also catalogued as HD 3651 b) is an extrasolar planet approximately 36 light-years away in the constellation of Pisces. It orbits the orange dwarf star 54 Piscium and is notable for its very eccentric orbit, which is perturbed by a brown dwarf in the same system.
Quick Facts
- Discoverer
- Fischer et al.
- Discovery Site
- Lick Observatory and Keck Observatory
- Discovered
- 2003
- Discovery Method
- Doppler spectroscopy
- Eccentricity
- 0.645 · 0.02
- Star
- 54 Piscium A
Facts from the source article.
Lore & Background
The planet was discovered on January 16, 2003, by a team led by Geoff Marcy using the radial velocity method, which detects the wobble of a star caused by an orbiting companion. Its mass is estimated at 20 percent of Jupiter, making it comparable to Saturn in size and mass. The planet orbits its star at 0.28 AU (within Mercury's orbit) and completes an orbit every 62 days. Its orbit has a high eccentricity of about 0.63, suggesting gravitational influence from an unseen object farther out. This was later explained by the discovery of a brown dwarf in the system. A 2006 simulation showed that 54 Piscium b's orbit sweeps clean most test particles within 0.5 AU, leaving only asteroids in low-eccentricity orbits near the planet's apastron distance and near the 1:2 mean-motion resonance. Observations have ruled out Neptune-class or heavier planets with a period of one year or less, but still allow for Earth-sized planets at 0.6 AU or more.
Reader's Guide
54 Piscium Ab is significant as an early radial-velocity discovery that highlighted the role of multiple bodies in shaping planetary orbits. Its high eccentricity, initially puzzling, was resolved by the detection of a brown dwarf in the system, demonstrating how unseen companions can perturb inner planets. The 2006 simulation further clarified the dynamical environment, showing that the planet's orbit clears most material within 0.5 AU, which constrains the possible locations of other planets. The system thus serves as a case study for how brown dwarfs influence planetary system architecture. The discovery also helped refine the radial velocity method for detecting low-mass planets, as 54 Piscium Ab's Saturn-like mass was near the detection limits at the time. Its legacy includes informing models of eccentricity excitation and orbital stability in multi-body systems.
Did You Know?
- 54 Piscium Ab has a minimum mass of one-fifth that of Jupiter, similar to Saturn.
- Its orbit is highly eccentric, with an eccentricity of about 0.63.
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