376 Geometria
A three-dimensional model of 376 Geometria based on its light curve | |
| Discovery[1] | |
|---|---|
| Discovered by | Auguste Charlois |
| Discovery site | Nice Observatory |
| Discovery date | 18 September 1893 |
| Designations | |
| (376) Geometria | |
| Pronunciation | /ˌdʒiːəˈmɛtriə, dʒiə-/ |
Named after | geometry |
| A893 SC · 1950 BQ1 · 1954 BJ[2][a] | |
| Main belt | |
| Orbital characteristics[2] | |
| Epoch 21 November 2025 (JD 2461000.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 126.70 yr (46278 d) |
| Aphelion | 2.68253 AU (401.301 Gm) |
| Perihelion | 1.89377 AU (283.304 Gm) |
| 2.28815 AU (342.302 Gm) | |
| Eccentricity | 0.172358 |
| 3.46126 yr (1264.23 d) | |
| 151.513° | |
| 0° 17m 5.132s / day | |
| Inclination | 5.43065° |
| 301.948° | |
| 316.527° | |
| Jupiter MOID | 2.3929 AU (357.97 Gm) |
| TJupiter | 3.575 |
| Physical characteristics | |
| 35.465 km[2] | |
| 7.7274600 ± 9.6×10−6 h (0.3219775 ± 0.0000004 d)[4]: 333 | |
Pole ecliptic longitude | 57±5° or 240±5°[4]: 333 |
Pole ecliptic latitude | −22±5° or −35±5°[4]: 333 |
| 0.321[2] | |
| S (Tholen) SI (SMASSII)[2] | |
| 9.49 | |
376 Geometria is an asteroid located within the main asteroid belt that was discovered by French astronomer Auguste Charlois on 18 September 1893 in Nice, France. It is classified as an S-type asteroid.[5] It is about 35.5 kilometres (22.1 mi) in size and has a rotation period of 7.73 hours.
History
Geometria was discovered by astronomer Auguste Charlois on 18 September 1893 at Nice Observatory.[1] Upon its discovery, it was given the old-style provisional designation 1893 AM, and by the next year it was assigned the permanent number (376).[3]: 241 On 23 August 1901,[6] it was named Geometria after the Latin word geometria, referring to the field of geometry.[7]: 44 Its name was announced by Johann Bauschinger alongside those of 33 other minor planets on the journal Astronomische Nachrichten, with the names having been selected by the Astronomical Calculation Institute.[7]: 43
In 1925, the old-style minor planet provisional designation scheme was replaced by the system currently in use. The Minor Planet Center (MPC) has since retroactively replaced old-style designations with new-style designations. [8] Thus, Geometria's provisional designation given upon its discovery was replaced by A893 SC.[2]
Orbit
Geometria orbits the Sun at an average distance—its semi-major axis—of 2.29 astronomical units (AU), taking 3.46 years to complete one revolution. Along its orbit, its distance from the Sun varies between 1.89 AU at perihelion to 2.68 AU at aphelion due to its orbital eccentricity of 0.17. Its orbit is inclined by 5.43° with respect to the ecliptic plane.[2]
Physical characteristics
Geometria has an estimated diameter of 35.5 kilometres (22.1 mi),[2] with a roughly spherical shape.[4]: 335 It is classified as an S-type asteroid in the Tholen classification scheme and an SI-type asteroid in the Small Main-belt Asteroid Spectroscopic Survey, Phase II (SMASSII) classification scheme. It has a geometric albedo of 0.321.[2]
Observations of Geometria's lightcurve, or variations in its observed brightness, show that it has a rotation period of 7.73 hours, accurately measured to within 0.035 seconds. It has a retrograde rotation, rotating backwards relative to its orbital direction with its rotational pole pointed towards the ecliptic south.[4]: 333 Determinations of Geometria's rotation period remained relatively consistent in the past, with 1983 observations from the Observatoire de Haute-Provence yielding a period of 7.74±0.02 hours and observations taken in November 1994 yielding a period of 7.734 hours.[5][4]: 332–333 However, past attempts at determining Geometria's spin orientation were ambiguous.[4]: 335
Notes
References
- ^ a b c "(376) Geometria = 1893 SC = 1950 BQ1 = 1954 BJ". Minor Planet Center. Archived from the original on 4 March 2016. Retrieved 23 November 2025. (7708 obs)
- ^ a b c d e f g h i Yeomans, Donald K., "376 Geometria", JPL Small-Body Database Browser, NASA Jet Propulsion Laboratory, archived from the original on 17 July 2021, retrieved 23 November 2025.
- ^ a b "Notes on some Points connected with the Progress of Astronomy during the Past Year". Monthly Notices of the Royal Astronomical Society. 54 (4): 240–267. 9 February 1894. doi:10.1093/mnras/54.4.240.
- ^ a b c d e f g Michałowski, T.; et al. (November 2005). "Photometry and models of selected main belt asteroids. II. 173 Ino, 376 Geometria, and 451 Patientia". Astronomy and Astrophysics. 443 (1): 329–335. Bibcode:2005A&A...443..329M. doi:10.1051/0004-6361:20053656. Archived from the original on 12 November 2024. Retrieved 17 February 2026.
- ^ a b Barucci, M. A.; di Martino, M. (July 1984), "Rotational rates of very small asteroids - 123 Brunhild, 376 Geometria, 437 Rhodia and 1224 Fantasia", Astronomy and Astrophysics Supplement Series, vol. 57, pp. 103–106, Bibcode:1984A&AS...57..103B, archived from the original on 4 December 2024, retrieved 17 February 2026.
- ^ Bauschinger, J. (23 August 1901). "Benennung von kleinen Planeten". Astronomische Nachrichten (in German). 156: 239. Bibcode:1901AN....156..239B. doi:10.1002/asna.19011561520.
- ^ a b Schmadel, Lutz D. (11 November 2013). Dictionary of Minor Planet Names. Vol. 2 (6 ed.). Springer Berlin, Heidelberg. p. 1452. doi:10.1007/978-3-642-29718-2. ISBN 978-3-642-29717-5.
- ^ "Provisional Designations". Minor Planets Center. Archived from the original on 11 July 2025. Retrieved 5 November 2025.
External links
- 376 Geometria at AstDyS-2, Asteroids—Dynamic Site
- 376 Geometria at the JPL Small-Body Database