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790 Pretoria

From Wikipedia, the free encyclopedia
Main-belt Asteroid

790 Pretoria
Discovery
Discovered byH. E. Wood
Discovery siteJohannesburg Observatory
Discovery date16 January 1912
Designations
(790) Pretoria
Pronunciation/prɪˈtɔːriə/[1]
1912 NW
Orbital characteristics[2]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc92.04 yr (33619 d)
Aphelion3.9279 AU (587.61 Gm)
Perihelion2.8955 AU (433.16 Gm)
3.4117 AU (510.38 Gm)
Eccentricity0.15130
6.30yr (2301.7d)
87.1149°
0° 9m 23.04s / day
Inclination20.526°
252.032°
38.637°
Physical characteristics
85.185±1.3km[2]
80.49 ± 5.58 km[3]
Mass(4.58 ± 0.28) × 1018 kg[3]
2.09 ± 0.45 g/cm3[3]
10.37 h (0.432 d)
0.0384±0.001
8.00

790 Pretoria is aminor planet orbiting theSun that was discovered by English astronomerHarry Edwin Wood on January 16, 1912. It is a member of theCybele group located beyond the core of themain belt[4] (seeMinor planet groups) and named afterPretoria, the capital city ofSouth Africa.

10μ radiometric data collected fromKitt Peak in 1975 gave a diameter estimate of 175 km.[5] In the present day it is estimated to be 170 km (106 mi) in diameter.[2]Photometric measurements of the asteroid made in 2005 at thePalmer Divide Observatory showed alight curve with a period of 10.370 ± 0.002 hours and a brightness variation of 0.08 ± 0.03 in magnitude.[6]

790 Pretoria has been observed tooccult 15 stars between 1998 and 2023.

References

[edit]
  1. ^"Pretoria".Dictionary.com Unabridged (Online). n.d.
  2. ^abc"JPL Small-Body Database Browser: 790 Pretoria (1912 NW)" (2009-12-21 last obs). Archived fromthe original on 10 June 2011. Retrieved4 May 2016.
  3. ^abcCarry, B. (December 2012), "Density of asteroids",Planetary and Space Science,73 (1):98–118,arXiv:1203.4336,Bibcode:2012P&SS...73...98C,doi:10.1016/j.pss.2012.03.009,S2CID 119226456. See Table 1.
  4. ^De Prá, M. N.; et al. (September 2018), "PRIMASS visits Hilda and Cybele groups",Icarus,311:35–51,arXiv:1711.02071,Bibcode:2018Icar..311...35D,doi:10.1016/j.icarus.2017.11.012,S2CID 119383924.
  5. ^Morrison, D.; Chapman, C. R. (March 1976), "Radiometric diameters for an additional 22 asteroids",Astrophysical Journal, vol. 204, pp. 934–939,Bibcode:2008mgm..conf.2594S,doi:10.1142/9789812834300_0469.
  6. ^Warner, Brian D. (2005), "Asteroid lightcurve analysis at the Palmer Divide Observatory - winter 2004-2005",The Minor Planet Bulletin,32 (3):54–58,Bibcode:2005MPBu...32...54W.

External links

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