Discovery [1] | |
---|---|
Discovered by | K. Reinmuth |
Discovery site | Heidelberg Obs. |
Discovery date | 9 January 1957 |
Designations | |
(2391) Tomita | |
Named after |
Kōichirō Tomita (Japanese astronomer) [2] |
1957 AA · 1929 VX 1938 BF · 1942 DF 1957 BA · 1977 KM 1978 PA4 · 1980 DC6 | |
main-belt · Nysa [3] | |
Orbital characteristics [1] | |
Epoch 4 September 2017 ( JD 2458000.5) | |
Uncertainty parameter 0 | |
Observation arc | 87.07 yr (31,804 days) |
Aphelion | 2.7676 AU |
Perihelion | 2.1141 AU |
2.4408 AU | |
Eccentricity | 0.1339 |
3.81 yr (1,393 days) | |
345.07 ° | |
0° 15m 30.6s / day | |
Inclination | 3.0111° |
163.32° | |
282.65° | |
Physical characteristics | |
Dimensions | 9.17 km (calculated)
[3] 15.07±4.33 km [4] 15.20±3.74 km [5] 16.62±0.23 km [6] 17.941±0.129 [7] 19.412±0.175 km [8] |
7.9533±0.0005
h
[a] 8.435±0.079 h [b] | |
0.0321±0.0044
[8] 0.06±0.03 [5] 0.070±0.004 [6] 0.07±0.07 [4] [7] 0.21 (assumed) [3] | |
S [3] · C [9] | |
12.4 [4] [6] [8] · 12.5 [1] [3] · 12.66 [5] · 12.74±0.28 [9] | |
2391 Tomita, provisional designation 1957 AA, is a Nysian asteroid from the inner regions of the asteroid belt, approximately 15 kilometers in diameter. The asteroid was discovered on 9 January 1957, by German astronomer Karl Reinmuth at Heidelberg Observatory in southern Germany. [10] It was named after Japanese astronomer Kōichirō Tomita. [2]
Tomita is a member of the Nysa family, which is named after its most massive member 44 Nysa. It orbits the Sun in the inner main-belt at a distance of 2.1–2.8 AU once every 3 years and 10 months (1,393 days). Its orbit has an eccentricity of 0.13 and an inclination of 3 ° with respect to the ecliptic. [1]
A first precovery was taken at Lowell Observatory in 1929, extending the body's observation arc by 28 years prior to its official discovery observation at Heidelberg. [10]
Tomita has been characterized as a stony S-type asteroid by the Collaborative Asteroid Lightcurve Link (CALL), and as a carbonaceous C-type asteroid by Pan-STARRS' photometric survey. [3] [9]
According to the surveys carried out by NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, the asteroid measures between 15.07 and 19.4 kilometers in diameter and its surface has a low albedo between 0.03 and 0.07, respectively. [4] [5] [6] [7] [8]
As CALL considers the body to be of a stony composition, it assumes a much higher albedo of 0.21 and calculates a diameter of 9.2 kilometers, as the higher the asteroid's reflectivity (albedo), the shorter its diameter at a constant absolute magnitude (brightness). [3]
In December 2013, two rotational lightcurves were obtained for this asteroid from photometric observations. They gave a rotation period of 7.9533±0.0005 and 8.435±0.079 hours with a brightness variation of 0.14 and 0.15 in magnitude, respectively. ( U=3/n.a.). [a] [b]
This minor planet was named in honor of Japanese astronomer Kōichirō Tomita (1925–2006), long-time observer at the Tokyo Astronomical Observatory, and a discoverer of minor planets and comets himself. Tomita was also known as one of Japan's principal popularizer of astronomy. [2] The official naming citation was published by the Minor Planet Center on 14 April 1987 ( M.P.C. 11748). [11]
Discovery [1] | |
---|---|
Discovered by | K. Reinmuth |
Discovery site | Heidelberg Obs. |
Discovery date | 9 January 1957 |
Designations | |
(2391) Tomita | |
Named after |
Kōichirō Tomita (Japanese astronomer) [2] |
1957 AA · 1929 VX 1938 BF · 1942 DF 1957 BA · 1977 KM 1978 PA4 · 1980 DC6 | |
main-belt · Nysa [3] | |
Orbital characteristics [1] | |
Epoch 4 September 2017 ( JD 2458000.5) | |
Uncertainty parameter 0 | |
Observation arc | 87.07 yr (31,804 days) |
Aphelion | 2.7676 AU |
Perihelion | 2.1141 AU |
2.4408 AU | |
Eccentricity | 0.1339 |
3.81 yr (1,393 days) | |
345.07 ° | |
0° 15m 30.6s / day | |
Inclination | 3.0111° |
163.32° | |
282.65° | |
Physical characteristics | |
Dimensions | 9.17 km (calculated)
[3] 15.07±4.33 km [4] 15.20±3.74 km [5] 16.62±0.23 km [6] 17.941±0.129 [7] 19.412±0.175 km [8] |
7.9533±0.0005
h
[a] 8.435±0.079 h [b] | |
0.0321±0.0044
[8] 0.06±0.03 [5] 0.070±0.004 [6] 0.07±0.07 [4] [7] 0.21 (assumed) [3] | |
S [3] · C [9] | |
12.4 [4] [6] [8] · 12.5 [1] [3] · 12.66 [5] · 12.74±0.28 [9] | |
2391 Tomita, provisional designation 1957 AA, is a Nysian asteroid from the inner regions of the asteroid belt, approximately 15 kilometers in diameter. The asteroid was discovered on 9 January 1957, by German astronomer Karl Reinmuth at Heidelberg Observatory in southern Germany. [10] It was named after Japanese astronomer Kōichirō Tomita. [2]
Tomita is a member of the Nysa family, which is named after its most massive member 44 Nysa. It orbits the Sun in the inner main-belt at a distance of 2.1–2.8 AU once every 3 years and 10 months (1,393 days). Its orbit has an eccentricity of 0.13 and an inclination of 3 ° with respect to the ecliptic. [1]
A first precovery was taken at Lowell Observatory in 1929, extending the body's observation arc by 28 years prior to its official discovery observation at Heidelberg. [10]
Tomita has been characterized as a stony S-type asteroid by the Collaborative Asteroid Lightcurve Link (CALL), and as a carbonaceous C-type asteroid by Pan-STARRS' photometric survey. [3] [9]
According to the surveys carried out by NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, the asteroid measures between 15.07 and 19.4 kilometers in diameter and its surface has a low albedo between 0.03 and 0.07, respectively. [4] [5] [6] [7] [8]
As CALL considers the body to be of a stony composition, it assumes a much higher albedo of 0.21 and calculates a diameter of 9.2 kilometers, as the higher the asteroid's reflectivity (albedo), the shorter its diameter at a constant absolute magnitude (brightness). [3]
In December 2013, two rotational lightcurves were obtained for this asteroid from photometric observations. They gave a rotation period of 7.9533±0.0005 and 8.435±0.079 hours with a brightness variation of 0.14 and 0.15 in magnitude, respectively. ( U=3/n.a.). [a] [b]
This minor planet was named in honor of Japanese astronomer Kōichirō Tomita (1925–2006), long-time observer at the Tokyo Astronomical Observatory, and a discoverer of minor planets and comets himself. Tomita was also known as one of Japan's principal popularizer of astronomy. [2] The official naming citation was published by the Minor Planet Center on 14 April 1987 ( M.P.C. 11748). [11]