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376 Geometria

From Wikipedia, the free encyclopedia
Main-belt asteroid

376 Geometria
A three-dimensional model of 376 Geometria based on its light curve
Discovery[1]
Discovered byAuguste Charlois
Discovery siteNice Observatory
Discovery date18 September 1893
Designations
(376) Geometria
Pronunciation/ˌəˈmɛtriə,iə-/
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 arc126.70 yr (46278 d)
Aphelion2.68253 AU (401.301 Gm)
Perihelion1.89377 AU (283.304 Gm)
2.28815 AU (342.302 Gm)
Eccentricity0.172358
3.46126yr (1264.23d)
151.513°
0° 17m 5.132s / day
Inclination5.43065°
301.948°
316.527°
Jupiter MOID2.3929 AU (357.97 Gm)
TJupiter3.575
Physical characteristics
35.465 km[2]
7.7274600 ± 9.6×10−6 h (0.3219775 ± 0.0000004 d)[4]: 333 
57± or240±[4]: 333 
−22± or−35±[4]: 333 
0.321[2]
S (Tholen)
SI (SMASSII)[2]
9.49

376 Geometria is anasteroid located within themain asteroid belt that was discovered by French astronomerAuguste Charlois on 18 September 1893 inNice, France. It is classified as anS-type asteroid.[5] It is about 35.5 kilometres (22.1 mi) in size and has arotation period of 7.73 hours.

History

[edit]

Geometria was discovered by astronomerAuguste Charlois on 18 September 1893 atNice Observatory.[1] Upon its discovery, it was given the old-styleprovisional designation1893 AM, and by the next year it was assigned the permanent number (376).[3]: 241  On 23 August 1901,[6] it was namedGeometria after the Latin wordgeometria, referring to the field ofgeometry.[7]: 44  Its name was announced byJohann Bauschinger alongside those of 33 other minor planets on the journalAstronomische Nachrichten, with the names having been selected by theAstronomical Calculation Institute.[7]: 43 

In 1925, the old-style minor planet provisional designation scheme was replaced by the system currently in use. TheMinor 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 byA893 SC.[2]

Orbit

[edit]

Geometria orbits the Sun at an average distance—itssemi-major axis—of 2.29astronomical units (AU), taking 3.46 years to complete one revolution. Along its orbit, its distance from the Sun varies between 1.89 AU atperihelion to 2.68 AU ataphelion due to itsorbital eccentricity of 0.17. Its orbit isinclined by 5.43° with respect to theecliptic plane.[2]

Physical characteristics

[edit]

Geometria has an estimated diameter of 35.5 kilometres (22.1 mi),[2] with a roughly spherical shape.[4]: 335  It is classified as anS-type asteroid in theTholen classification scheme and anSI-type asteroid in theSmall Main-belt Asteroid Spectroscopic Survey, Phase II (SMASSII) classification scheme. It has ageometric albedo of 0.321.[2]

Observations of Geometria'slightcurve, or variations in its observed brightness, show that it has arotation period of 7.73 hours, accurately measured to within 0.035 seconds. It has aretrograde rotation, rotating backwards relative to its orbital direction with its rotational pole pointed towards theecliptic south.[4]: 333  Determinations of Geometria's rotation period remained relatively consistent in the past, with 1983 observations from theObservatoire de Haute-Provence yielding a period of7.74±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

[edit]
  1. ^The MPC notates Geometria's retroactively applied designation as1893 SC.[1] Its old-style designation was1893 AM.[3]: 241 

References

[edit]
  1. ^abc"(376) Geometria = 1893 SC = 1950 BQ1 = 1954 BJ". Minor Planet Center. Retrieved23 November 2025.{{cite web}}: CS1 maint: url-status (link) (7708 obs)
  2. ^abcdefghiYeomans, Donald K.,"376 Geometria",JPL Small-Body Database Browser,NASA Jet Propulsion Laboratory, retrieved23 November 2025.
  3. ^ab"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.
  4. ^abcdefgMichałowski, 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.
  5. ^abBarucci, 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.
  6. ^Bauschinger, J. (23 August 1901). "Benennung von kleinen Planeten".Astronomische Nachrichten (in German).156: 239.Bibcode:1901AN....156..239B.doi:10.1002/asna.19011561520.
  7. ^abSchmadel, 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.
  8. ^"Provisional Designations". Minor Planets Center. Archived fromthe original on 11 July 2025. Retrieved5 November 2025.

External links

[edit]
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Asteroid
Distant minor planet
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