-based 3D model of
Amphitrite Amphitrite's orbit is less eccentric and inclined than those of its larger cousins; indeed, it is the most circular of any asteroid discovered up to that point. As a consequence, it never becomes as bright as Iris or
Hebe, especially as it is much further from the Sun than those asteroids. It can reach magnitudes of around +8.6 at a favorable opposition, but usually is around the
binocular limit of +9.5. In 2007, James Baer and Steven R. Chesley estimated Amphitrite to have a mass of 1.9 kg. A 2008 estimate by Baer suggests it has a mass of 1.18 kg. A
satellite of the asteroid is suspected to exist, based on lightcurve data collected by Edward F. Tedesco. In 1988 a search for satellites or dust orbiting this asteroid was performed using the
UH88 telescope at the
Mauna Kea Observatories, but neither were found. == Proposed exploration ==