Discovery [1] | |
---|---|
Discovered by | T. Gehrels |
Discovery site | Palomar Obs. |
Discovery date | 15 September 1972 |
Designations | |
(5040) Rabinowitz | |
Named after |
David Rabinowitz (American astronomer) [2] |
1972 RF · 1987 QE | |
main-belt · Phocaea [3] [4] | |
Orbital characteristics [1] | |
Epoch 4 September 2017 ( JD 2458000.5) | |
Uncertainty parameter 0 | |
Observation arc | 46.20 yr (16,874 days) |
Aphelion | 2.9644 AU |
Perihelion | 1.8705 AU |
2.4174 AU | |
Eccentricity | 0.2263 |
3.76 yr (1,373 days) | |
7.0892 ° | |
0° 15m 43.92s / day | |
Inclination | 24.361° |
175.69° | |
149.71° | |
Physical characteristics | |
Dimensions | 6.41 km (calculated) [3] |
4.472±0.001
h
[5] 4.6901±0.0004 h [a] 4.691±0.001 h [6] | |
0.23 (assumed) [3] | |
S [3] | |
12.73±0.13 (R) [a] · 12.9 [1] · 13.15±0.35 [7] · 13.18 [3] | |
5040 Rabinowitz, provisional designation 1972 RF, is a stony Phocaea asteroid from the inner regions of the asteroid belt, approximately 6 kilometers in diameter. It was discovered by Dutch–American astronomer Tom Gehrels at Palomar Observatory on 15 September 1972. [8] Contrary to most of his discoveries, this asteroid is unrelated to the Palomar–Leiden survey and exclusively credited to Tom Gehrels.
The stony S-type asteroid is a member of the Phocaea family ( 701), a group of asteroids with similar orbital characteristics, named after its largest member, 25 Phocaea. [4] It orbits the Sun in the inner main-belt at a distance of 1.9–3.0 AU once every 3 years and 9 months (1,373 days). Its orbit has an eccentricity of 0.23 and an inclination of 24 ° with respect to the ecliptic. [1] A first precovery was taken at the discovering observatory in 1971, extending the body's observation arc by one year prior to its official discovery observation. [8]
In July 2013, a rotational lightcurve for this asteroid was obtained from photometric observations by Czech astronomer Petr Pravec at the Ondřejov Observatory. The well-defined lightcurve gave a rotation period of 4.6901±0.0004 hours with a brightness variation of 0.33 in magnitude ( U=3). [a]
During the same opposition opportunity, two more lightcurves – obtained by Robert Stephens at the Center for Solar System Studies and by Maurice Clark at the Preston Gott Observatory – gave a similar period of 4.691 and 4.472 hours, with an amplitude of 0.35 and 0.31 in magnitude, respectively ( U=3-/2+). [5] [6]
The Collaborative Asteroid Lightcurve Link assumes an albedo of 0.23, derived from the Phocaea family's namesake, and calculates a diameter of 6.4 kilometers with an absolute magnitude of 13.18. [3]
This minor planet was named after American astronomer David Rabinowitz (born 1960), a discoverer of minor planets himself and researcher at Yale University. The naming also honors his work for the Spacewatch program. [2] The official naming citation was published by the Minor Planet Center on 1 September 1993 ( M.P.C. 22505). [9]
Discovery [1] | |
---|---|
Discovered by | T. Gehrels |
Discovery site | Palomar Obs. |
Discovery date | 15 September 1972 |
Designations | |
(5040) Rabinowitz | |
Named after |
David Rabinowitz (American astronomer) [2] |
1972 RF · 1987 QE | |
main-belt · Phocaea [3] [4] | |
Orbital characteristics [1] | |
Epoch 4 September 2017 ( JD 2458000.5) | |
Uncertainty parameter 0 | |
Observation arc | 46.20 yr (16,874 days) |
Aphelion | 2.9644 AU |
Perihelion | 1.8705 AU |
2.4174 AU | |
Eccentricity | 0.2263 |
3.76 yr (1,373 days) | |
7.0892 ° | |
0° 15m 43.92s / day | |
Inclination | 24.361° |
175.69° | |
149.71° | |
Physical characteristics | |
Dimensions | 6.41 km (calculated) [3] |
4.472±0.001
h
[5] 4.6901±0.0004 h [a] 4.691±0.001 h [6] | |
0.23 (assumed) [3] | |
S [3] | |
12.73±0.13 (R) [a] · 12.9 [1] · 13.15±0.35 [7] · 13.18 [3] | |
5040 Rabinowitz, provisional designation 1972 RF, is a stony Phocaea asteroid from the inner regions of the asteroid belt, approximately 6 kilometers in diameter. It was discovered by Dutch–American astronomer Tom Gehrels at Palomar Observatory on 15 September 1972. [8] Contrary to most of his discoveries, this asteroid is unrelated to the Palomar–Leiden survey and exclusively credited to Tom Gehrels.
The stony S-type asteroid is a member of the Phocaea family ( 701), a group of asteroids with similar orbital characteristics, named after its largest member, 25 Phocaea. [4] It orbits the Sun in the inner main-belt at a distance of 1.9–3.0 AU once every 3 years and 9 months (1,373 days). Its orbit has an eccentricity of 0.23 and an inclination of 24 ° with respect to the ecliptic. [1] A first precovery was taken at the discovering observatory in 1971, extending the body's observation arc by one year prior to its official discovery observation. [8]
In July 2013, a rotational lightcurve for this asteroid was obtained from photometric observations by Czech astronomer Petr Pravec at the Ondřejov Observatory. The well-defined lightcurve gave a rotation period of 4.6901±0.0004 hours with a brightness variation of 0.33 in magnitude ( U=3). [a]
During the same opposition opportunity, two more lightcurves – obtained by Robert Stephens at the Center for Solar System Studies and by Maurice Clark at the Preston Gott Observatory – gave a similar period of 4.691 and 4.472 hours, with an amplitude of 0.35 and 0.31 in magnitude, respectively ( U=3-/2+). [5] [6]
The Collaborative Asteroid Lightcurve Link assumes an albedo of 0.23, derived from the Phocaea family's namesake, and calculates a diameter of 6.4 kilometers with an absolute magnitude of 13.18. [3]
This minor planet was named after American astronomer David Rabinowitz (born 1960), a discoverer of minor planets himself and researcher at Yale University. The naming also honors his work for the Spacewatch program. [2] The official naming citation was published by the Minor Planet Center on 1 September 1993 ( M.P.C. 22505). [9]