Discovery [1] | |
---|---|
Discovered by | J. E. Mueller |
Discovery site | Palomar Obs. |
Discovery date | 23 August 1987 |
Designations | |
(4257) Ubasti | |
Named after |
Bastet
[2] (Egyptian goddess of cats) |
1987 QA | |
NEO ·
Apollo
[1]
[3] Mars-crosser | |
Orbital characteristics [1] | |
Epoch 4 September 2017 ( JD 2458000.5) | |
Uncertainty parameter 0 | |
Observation arc | 29.02 yr (10,600 days) |
Aphelion | 2.4183 AU |
Perihelion | 0.8759 AU |
1.6471 AU | |
Eccentricity | 0.4682 |
2.11 yr (772 days) | |
28.670 ° | |
0° 27m 58.32s / day | |
Inclination | 40.716° |
169.22° | |
278.92° | |
Earth MOID | 0.1714 AU · 66.8 LD |
Physical characteristics | |
Dimensions | 1.30±0.09 km
[4] 1.96 km (calculated) [5] |
0.20 (assumed)
[5] 0.376±0.053 [4] | |
S [5] | |
15.9 [1] [5] · 16.20 [4] | |
4257 Ubasti, provisional designation 1987 QA, is a stony asteroid, classified as near-Earth object of the Apollo group and as Mars-crosser, approximately 1.5 kilometers in diameter. It was discovered by American astronomer Jean Mueller at the Palomar Observatory in California on 23 August 1987. [3] The asteroid was named for Bastet – also known as Baast, Ubaste or Ubasti – the Egyptian goddess of cats. [2]
Ubasti orbits the Sun at a distance of 0.9–2.4 AU once every 2 years and 1 month (772 days). Its orbit has an eccentricity of 0.47 and an inclination of 41 ° with respect to the ecliptic. [1] Due to its high eccentricity, Ubasti is also a Mars-crossing asteroid. The body's observation arc begins with its official discovery observation, as no precoveries were taken and no prior identification had been made. [3]
As a near-Earth object, Ubasti has a low Earth minimum orbital intersection distance of 0.1714 AU (25,600,000 km), which corresponds to 66.8 lunar distances (LD). This distance, however, is too large to make it a potentially hazardous asteroid (0.05 AU; less than 20 LD). [1]
Ubasti is an assumed stony S-type asteroid. [5]
As of 2017, no rotational lightcurve of Ubasti has been obtained and its rotation period remains unknown. [5] However, the Lowell Observatory Near-Earth Asteroid Photometric Survey has measured the body's brightness variation caused by its rotation, which gave a maximum of 0.36 magnitude. This indicates that the body has a somewhat non-spherical shape. [6]
According to the survey carried out by the Japanese Akari satellite, Ubasti measures 1.30 kilometers in diameter and its surface has an albedo of 0.376, [4] while the Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 1.96 kilometers based on an absolute magnitude of 15.9. [5]
This minor planet was named after Egyptian goddesses Bastet, who was originally the goddess of warfare, equated with the lioness war goddess, but later transformed into a major protector deity represented as a cat. [2] The official naming citation was published by the Minor Planet Center on 21 November 1991 ( M.P.C. 19336). [7] The discoverer dedicated this asteroid to her beloved companion, Pepper Cat (1974–1991). [2]
Discovery [1] | |
---|---|
Discovered by | J. E. Mueller |
Discovery site | Palomar Obs. |
Discovery date | 23 August 1987 |
Designations | |
(4257) Ubasti | |
Named after |
Bastet
[2] (Egyptian goddess of cats) |
1987 QA | |
NEO ·
Apollo
[1]
[3] Mars-crosser | |
Orbital characteristics [1] | |
Epoch 4 September 2017 ( JD 2458000.5) | |
Uncertainty parameter 0 | |
Observation arc | 29.02 yr (10,600 days) |
Aphelion | 2.4183 AU |
Perihelion | 0.8759 AU |
1.6471 AU | |
Eccentricity | 0.4682 |
2.11 yr (772 days) | |
28.670 ° | |
0° 27m 58.32s / day | |
Inclination | 40.716° |
169.22° | |
278.92° | |
Earth MOID | 0.1714 AU · 66.8 LD |
Physical characteristics | |
Dimensions | 1.30±0.09 km
[4] 1.96 km (calculated) [5] |
0.20 (assumed)
[5] 0.376±0.053 [4] | |
S [5] | |
15.9 [1] [5] · 16.20 [4] | |
4257 Ubasti, provisional designation 1987 QA, is a stony asteroid, classified as near-Earth object of the Apollo group and as Mars-crosser, approximately 1.5 kilometers in diameter. It was discovered by American astronomer Jean Mueller at the Palomar Observatory in California on 23 August 1987. [3] The asteroid was named for Bastet – also known as Baast, Ubaste or Ubasti – the Egyptian goddess of cats. [2]
Ubasti orbits the Sun at a distance of 0.9–2.4 AU once every 2 years and 1 month (772 days). Its orbit has an eccentricity of 0.47 and an inclination of 41 ° with respect to the ecliptic. [1] Due to its high eccentricity, Ubasti is also a Mars-crossing asteroid. The body's observation arc begins with its official discovery observation, as no precoveries were taken and no prior identification had been made. [3]
As a near-Earth object, Ubasti has a low Earth minimum orbital intersection distance of 0.1714 AU (25,600,000 km), which corresponds to 66.8 lunar distances (LD). This distance, however, is too large to make it a potentially hazardous asteroid (0.05 AU; less than 20 LD). [1]
Ubasti is an assumed stony S-type asteroid. [5]
As of 2017, no rotational lightcurve of Ubasti has been obtained and its rotation period remains unknown. [5] However, the Lowell Observatory Near-Earth Asteroid Photometric Survey has measured the body's brightness variation caused by its rotation, which gave a maximum of 0.36 magnitude. This indicates that the body has a somewhat non-spherical shape. [6]
According to the survey carried out by the Japanese Akari satellite, Ubasti measures 1.30 kilometers in diameter and its surface has an albedo of 0.376, [4] while the Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 1.96 kilometers based on an absolute magnitude of 15.9. [5]
This minor planet was named after Egyptian goddesses Bastet, who was originally the goddess of warfare, equated with the lioness war goddess, but later transformed into a major protector deity represented as a cat. [2] The official naming citation was published by the Minor Planet Center on 21 November 1991 ( M.P.C. 19336). [7] The discoverer dedicated this asteroid to her beloved companion, Pepper Cat (1974–1991). [2]