 VLT image of Amphitrite | |
| Discovery[1] | |
|---|---|
| Discovered by | A. Marth |
| Discovery site | London |
| Discovery date | 1 March 1854 |
| Designations | |
| (29) Amphitrite | |
| Pronunciation | /æmfɪˈtraɪtiː/[2] |
Named after | Amphitrite[3] (Greek mythology) |
| A899 NG | |
| main-belt[1][4] · (middle) background[5][6] | |
| Adjectives | Amphitritean/ˌæmfɪtrɪˈtiːən/,/ˌæmfɪˈtraɪtiən/ |
| Symbol | .svg) (historical) |
| Orbital characteristics[4] | |
| Epoch 17.0 October 2024 (JD 2460600.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 169.16yr (61,784 d) |
| Aphelion | 2.7425AU |
| Perihelion | 2.3664 AU |
| 2.5544 AU | |
| Eccentricity | 0.0736 |
| 4.08 yr (1491 d) | |
| 48.40° | |
| 0° 14m 29.04s / day | |
| Inclination | 6.0772° |
| 356.26° | |
| 62.01° | |
| Earth MOID | 1.38454 AU |
| Jupiter MOID | 2.48544 AU |
| TJupiter | 3.427 |
| Physical characteristics | |
| Dimensions | 233 km × 212 km × 193 km[7] 222 km × 209 km × 183 km (±6 km × 6 km × 5 km) |
| 204±2 km[8] 189.6±1.1 km[9] 196±22 km[10] 206.86 km[11] 212.22±6.8 km[12] 227.1±4.0 km[13] | |
| Flattening | 0.18[a] |
| Mass | (12.7±2.0)×1018 kg[8] (11.8 ± ?)×1018 kg[7] |
Meandensity | 2.86±0.45 g/cm3[8] 2.36±0.26 g/cm3[7] |
| 5.3921 h[14][6][4] 5.390119 ± 0.000001 h[8] | |
| 116°[8] | |
| 323°±2°[8] | |
| −29°±2°[8] | |
| 0.194[8] 0.157±0.035[13] 0.1793±0.012[12] 0.195[11] 0.216±0.043[9][4] | |
| S[6][4] | |
| 5.85[1] 5.98[4] 6.0[5] | |
29 Amphitrite is one of the largestS-type asteroids, approximately 200 kilometers (120 miles) in diameter, and probably fifth largest afterEunomia,Juno,Iris andHerculina.
Amphitrite was discovered byAlbert Marth on 1 March 1854, at the privateSouth Villa Observatory, inRegent's Park,London. It was Marth's only asteroid discovery. Its name was chosen by George Bishop, the owner of the observatory, who named it afterAmphitrite, a sea goddess inGreek mythology.[3] Its historical symbol was a shell and star; it was encoded inUnicode 17.0 as U+1CECF (.svg)
).[15][16]
.png)
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 orHebe, 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 thebinocular limit of +9.5.
In 2007, James Baer and Steven R. Chesley estimated Amphitrite to have a mass of 1.9×1019 kg.[17] A 2008 estimate by Baer suggests it has a mass of 1.18×1019 kg.[7]
Asatellite of the asteroid is suspected to exist, based on lightcurve data collected by Edward F. Tedesco.[18][19] In 1988 a search for satellites or dust orbiting this asteroid was performed using theUH88 telescope at theMauna Kea Observatories, but neither were found.[20]
In 1984, while determining theGalileo mission's prelaunch trajectory toJupiter, JPL engineers found out that if the spacecraft launched onMay 1986, it could perform a flyby of 29 Amphitrite at a distance of 6,200 mi (10,000 km) on 6 December 1986. However, with theChallenger disaster delaying the launch toOctober 1989, the flyby was ultimately cancelled.[21]
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