2634 James Bradley Notae | Nexus externi | Tabula navigationis"Discovery Circumstances: Numbered Minor Planets"2002634Small-Body Database

L +1Latinitas +1 (bona)Asteroides anno 1982 repertiAsteroides Cinguli Principalis Exterioris


asteroidessystematis solarisasteroidibus Cinguli Principalis ExteriorisAstronomismagnitudinem absolutam21 Februarii1982Edwardo BowellStationem Anderson Mesa (Observatorium Lowell)epochaeunitatum astronomicarumquam minimequam maximeInclinatio orbitalis°anomalia mediaP literature.svg[1]Small-Body DatabaseMercuriusVenusTellus (Terra)MarsIuppiterSaturnusUranusNeptunusSatellitesLunaAsteroidesindicesCorpora transneptuniana








































2634 James Bradley



Genus

Asteroides Cinguli Principalis Exterioris
Res orbitales epochae 4 Ianuarii 2010

Excentricitas
0.0535413

Axis semimaior

perihelion
aphelion

3.4510703 UA
3.2662955 UA
3.6358451 UA


Inclinatio orbitalis
6.40381°

Longitudo nodi ascendentis
133.75165°

Argumentum perihelii
343.17761°

Anomalia media
142.81891°

Periodus orbitalis
6.4111937612594 anni
Res physicae

Diameter

km

Massa

kg

Densitas media
g/cm3

Periodus rotationis

h m

Classis spectralis

Tholen
SMASS



—
—


Magnitudo absoluta
10.20

Albedo
0.0923
De recognitione
Primus repertor

E. Bowell
Repertum
die 21 Februarii 1982
Designationes aliae
1982 DL, 1931 FL, 1961 XH, 1963 FC, 1975 AO, 1976 GB1, 1977 KP, A905 CC

2634 James Bradley,[1] olim designationibus 1982 DL, 1931 FL, 1961 XH, 1963 FC, 1975 AO, 1976 GB1, 1977 KP, et A905 CC agnitus, est asteroides systematis solaris nostri, asteroidibus Cinguli Principalis Exterioris attributus. Astronomis terrestribus magnitudinem absolutam 10.20 monstrat. Die 21 Februarii 1982 ab Edwardo Bowell, astronomo apud Stationem Anderson Mesa (Observatorium Lowell) versato, repertus est.[2]


Rerum orbitalium ratio epochae 4 Ianuarii 2010 constitit. Qua epocha 2634 James Bradley per dies 2342 circa solem movebatur. Axem orbitalem habebat unitatum astronomicarum 3.45 et eccentricitatem 0.05, distans igitur a sole quam minime unitatibus 3.27, quam maxime unitatibus 3.64. Inclinatio orbitalis 6.4° reperiebatur, anomalia media 142.82°.



Notae |



  1. ↑ Nomina asteroidum iussu Unionis Astronomicae Internationalis imposita sunt.


  2. ↑ "Discovery Circumstances: Numbered Minor Planets" .mw-parser-output .existinglinksgray a,.mw-parser-output .existinglinksgray a:visitedcolor:gray.mw-parser-output .existinglinksgray a.newcolor:#ba0000.mw-parser-output .existinglinksgray a.new:visitedcolor:#a55858
    (Anglice). IAU Minor Planet Center. Universitas Harvardiana 



Nexus externi |





Wikidata-logo.svg
Data astronomica: "2002634" apud JPL Small-Body Database.

P literature.svgHaec commentatio, automatice praeparata, res astronomicas colligit excerptas e pagina [1] sitús Small-Body Database, quem elaboraverunt NASA et JPL apud Institutum Technologiae Californiense.






Systema Solare nostrum



SolMercuriusVenusLunaTellus/TerraMarsPhobos et DeimosCeresCingulus asteroidum principalisIuppiterSatellites IuppiterisAnuli IuppiterisSaturnusSatellites SaturniAnuli SaturniUranusSatellites UraniAnuli UraniNeptunusSatellites NeptuniAnuli NeptuniPlutoSatellites PlutonisHaumeaSatellites HaumeaeMakemakeZona KuiperiErisDysnomiaDiscus RarusNubes HillsNubes OortSolar System Template Final.png


Sol

Planetae: Mercurius | Venus | Tellus (Terra) | Mars | Iuppiter | Saturnus | Uranus | Neptunus



Planetulae: Ceres | Pluto | Haumea | Makemake | Eris

Corpora alia: Satellites | Luna | Asteroides (+ indices) | Corpora transneptuniana


Vide etiam indices corporum Systematis Solaris redactos secundum radium et massam.
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