Discovery[1][2] | |
---|---|
Discovered by | L. Chernykh |
Discovery site | Crimean Astrophysical Obs. |
Discovery date | 8 October 1969 |
Designations | |
(10001) Palermo | |
Named after | Palermo (Italian city)[1] |
1969 TM1 · 1991 RS27 | |
main-belt[1][3] · (inner) Vestian[4][5] | |
Orbital characteristics[3] | |
Epoch 23 March 2018 (JD 2458200.5) | |
Uncertainty parameter 0 | |
Observation arc | 63.50 yr (23,192 d) |
Aphelion | 2.6955 AU |
Perihelion | 2.0579 AU |
2.3767 AU | |
Eccentricity | 0.1341 |
3.66 yr (1,338 d) | |
66.907° | |
0° 16m 8.4s / day | |
Inclination | 7.4247° |
40.160° | |
357.81° | |
Physical characteristics | |
4.123±0.657 km[6] 4.31 km (calculated)[4] | |
213.368±2.0136 h[7] | |
0.20 (assumed)[4] 0.341±0.134[6] | |
S (assumed)[4] | |
13.71±0.42[8] 13.745±0.006 (R)[7] 13.80[6] · 13.9[3] · 14.19[4] | |
10001 Palermo, provisional designation 1969 TM1, is a Vestian asteroid and a slow rotator from the inner regions of the asteroid belt, approximately 4 kilometers (2.5 miles) in diameter. It was discovered on 8 October 1969, by Soviet–Russian astronomer Lyudmila Chernykh using a 0.4-meter double astrograph at the Crimean Astrophysical Observatory in Nauchnij on the Crimean peninsula.[2] The asteroid is likely elongated in shape and has a long rotation period of 213 hours.[4] It was named for the Italian city of Palermo to commemorate the discovery of Ceres two hundred years earlier.[1]
MPC-object
was invoked but never defined (see the help page).Chernykh-2002
was invoked but never defined (see the help page).jpldata
was invoked but never defined (see the help page).lcdb
was invoked but never defined (see the help page).Ferret
was invoked but never defined (see the help page).Nugent-2015
was invoked but never defined (see the help page).Waszczak-2015
was invoked but never defined (see the help page).Veres-2015
was invoked but never defined (see the help page).