Discovery [1] | |
---|---|
Discovered by |
C. Shoemaker E. Shoemaker |
Discovery site | Palomar Obs. |
Discovery date | 23 October 1984 |
Designations | |
(3700) Geowilliams | |
Named after |
George E. Williams
[1] (Australian geologist) |
1984 UL2 · 1973 YF2 1977 UJ | |
main-belt
[1]
[2] · (
inner)
[3] background [4] | |
Orbital characteristics [2] | |
Epoch 23 March 2018 ( JD 2458200.5) | |
Uncertainty parameter 0 | |
Observation arc | 43.54 yr (15,902 d) |
Aphelion | 2.9602 AU |
Perihelion | 1.8695 AU |
2.4148 AU | |
Eccentricity | 0.2258 |
3.75 yr (1,371 d) | |
293.18 ° | |
0° 15m 45.36s / day | |
Inclination | 12.121° |
289.16° | |
153.06° | |
Physical characteristics | |
7.712±0.130
km
[5] 7.74±1.83 km [6] 7.753±0.152 km [7] 8.70±0.30 km [8] 8.82±0.86 km [9] 8.97 km (calculated) [3] | |
14.383±0.0183
h
[10] 14.387±0.003 h [a] | |
0.20 (assumed)
[3] 0.227±0.045 [9] 0.23±0.13 [6] 0.233±0.033 [8] 0.2970±0.0516 [5] | |
SMASS = S k [2] | |
12.443±0.002 (R)
[10] 12.50 [5] [8] [9] 12.6 [2] [3] 12.89 [6] 12.94±0.46 [11] | |
3700 Geowilliams, provisional designation 1984 UL2, is a stony background asteroid from the inner regions of the asteroid belt, approximately 8 kilometers (5 miles) in diameter. It was discovered on 23 October 1984, by American astronomer couple Carolyn and Eugene Shoemaker at the Palomar Observatory in California, United States. [1] The S k-subtype has a rotation period of 14.38 hours. It was named for Australian geologist George E. Williams. [1]
Geowilliams is a non- family asteroid from the main belt's background population. [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 (1,371 days; semi-major axis of 2.41 AU). Its orbit has an eccentricity of 0.23 and an inclination of 12 ° with respect to the ecliptic. [2] The body's observation arc begins with its first observation as 1973 YF2 at Crimea-Nauchnij in December 1973, almost 11 years prior to its official discovery observation at Palomar. [1]
In the SMASS classification, Geowilliams is a Sk-subtype that transitions between the common S-type asteroid and the K-type asteroid. The latter spectral type is often found among members of the Eos family. [2]
In January 2008, a rotational lightcurve of Geowilliams was obtained from photometric observations by Australian amateur astronomer David Higgins at the Hunters Hill Observatory ( E14). Lightcurve analysis gave a well-defined rotation period of 14.387 hours with a brightness variation of 0.40 magnitude ( U=3). [a] In July 2010, a similar period of 14.383 hours and an amplitude of 0.42 was measured at the Palomar Transient Factory in California ( U=2). [10]
According to the surveys carried out by the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Geowilliams measures between 7.712 and 8.82 kilometers in diameter and its surface has an albedo between 0.227 and 0.297. [5] [6] [7] [8] [9]
The Collaborative Asteroid Lightcurve Link assumes a standard albedo for a stony asteroid of 0.20, and calculates a diameter of 8.97 kilometers based on an absolute magnitude of 12.6. [3]
This minor planet was named after Australian geologist George E. Williams who discovered the Acraman crater when he worked for BHP in South Australia. The old 90-kilometer impact structure is one of the largest meteorite impact craters known on Earth and the largest one on the Australian continent. [1] The official naming citation was published by the Minor Planet Center on 2 February 1988 ( M.P.C. 12810). [12]
Discovery [1] | |
---|---|
Discovered by |
C. Shoemaker E. Shoemaker |
Discovery site | Palomar Obs. |
Discovery date | 23 October 1984 |
Designations | |
(3700) Geowilliams | |
Named after |
George E. Williams
[1] (Australian geologist) |
1984 UL2 · 1973 YF2 1977 UJ | |
main-belt
[1]
[2] · (
inner)
[3] background [4] | |
Orbital characteristics [2] | |
Epoch 23 March 2018 ( JD 2458200.5) | |
Uncertainty parameter 0 | |
Observation arc | 43.54 yr (15,902 d) |
Aphelion | 2.9602 AU |
Perihelion | 1.8695 AU |
2.4148 AU | |
Eccentricity | 0.2258 |
3.75 yr (1,371 d) | |
293.18 ° | |
0° 15m 45.36s / day | |
Inclination | 12.121° |
289.16° | |
153.06° | |
Physical characteristics | |
7.712±0.130
km
[5] 7.74±1.83 km [6] 7.753±0.152 km [7] 8.70±0.30 km [8] 8.82±0.86 km [9] 8.97 km (calculated) [3] | |
14.383±0.0183
h
[10] 14.387±0.003 h [a] | |
0.20 (assumed)
[3] 0.227±0.045 [9] 0.23±0.13 [6] 0.233±0.033 [8] 0.2970±0.0516 [5] | |
SMASS = S k [2] | |
12.443±0.002 (R)
[10] 12.50 [5] [8] [9] 12.6 [2] [3] 12.89 [6] 12.94±0.46 [11] | |
3700 Geowilliams, provisional designation 1984 UL2, is a stony background asteroid from the inner regions of the asteroid belt, approximately 8 kilometers (5 miles) in diameter. It was discovered on 23 October 1984, by American astronomer couple Carolyn and Eugene Shoemaker at the Palomar Observatory in California, United States. [1] The S k-subtype has a rotation period of 14.38 hours. It was named for Australian geologist George E. Williams. [1]
Geowilliams is a non- family asteroid from the main belt's background population. [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 (1,371 days; semi-major axis of 2.41 AU). Its orbit has an eccentricity of 0.23 and an inclination of 12 ° with respect to the ecliptic. [2] The body's observation arc begins with its first observation as 1973 YF2 at Crimea-Nauchnij in December 1973, almost 11 years prior to its official discovery observation at Palomar. [1]
In the SMASS classification, Geowilliams is a Sk-subtype that transitions between the common S-type asteroid and the K-type asteroid. The latter spectral type is often found among members of the Eos family. [2]
In January 2008, a rotational lightcurve of Geowilliams was obtained from photometric observations by Australian amateur astronomer David Higgins at the Hunters Hill Observatory ( E14). Lightcurve analysis gave a well-defined rotation period of 14.387 hours with a brightness variation of 0.40 magnitude ( U=3). [a] In July 2010, a similar period of 14.383 hours and an amplitude of 0.42 was measured at the Palomar Transient Factory in California ( U=2). [10]
According to the surveys carried out by the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Geowilliams measures between 7.712 and 8.82 kilometers in diameter and its surface has an albedo between 0.227 and 0.297. [5] [6] [7] [8] [9]
The Collaborative Asteroid Lightcurve Link assumes a standard albedo for a stony asteroid of 0.20, and calculates a diameter of 8.97 kilometers based on an absolute magnitude of 12.6. [3]
This minor planet was named after Australian geologist George E. Williams who discovered the Acraman crater when he worked for BHP in South Australia. The old 90-kilometer impact structure is one of the largest meteorite impact craters known on Earth and the largest one on the Australian continent. [1] The official naming citation was published by the Minor Planet Center on 2 February 1988 ( M.P.C. 12810). [12]