3467 Bernheim Notae | Nexus externi | Tabula navigationis"Discovery Circumstances: Numbered Minor Planets"2003467Small-Body Database

L +1Latinitas +1 (bona)Asteroides anno 1981 repertiAsteroides Cinguli Principalis


asteroidessystematis solarisasteroidibus Cinguli PrincipalisAstronomismagnitudinem absolutam26 Septembris1981Normanno G. ThomasStationem Anderson Mesa (Observatorium Lowell)epochaeunitatum astronomicarumquam minimequam maximeInclinatio orbitalis°anomalia mediaP literature.svg[1]Small-Body DatabaseMercuriusVenusTellus (Terra)MarsIuppiterSaturnusUranusNeptunusSatellitesLunaAsteroidesindicesCorpora transneptuniana








































3467 Bernheim



Genus

Asteroides Cinguli Principalis
Res orbitales epochae 4 Ianuarii 2010

Excentricitas
0.1496956

Axis semimaior

perihelion
aphelion

2.4088931 UA
2.0482924 UA
2.7694938 UA


Inclinatio orbitalis
4.11204°

Longitudo nodi ascendentis
105.42304°

Argumentum perihelii
349.31559°

Anomalia media
124.37248°

Periodus orbitalis
3.7388194825462 anni
Res physicae

Diameter

km

Massa

kg

Densitas media
g/cm3

Periodus rotationis

h m

Classis spectralis

Tholen
SMASS






Magnitudo absoluta
13.0

Albedo
0.0448
De recognitione
Primus repertor

N. G. Thomas
Repertum
die 26 Septembris 1981
Designationes aliae
1981 SF2, 1929 WG1, 1949 BU, 1968 DP, 1970 WR, 1977 QJ, 1981 SJ6, 1981 UB19

3467 Bernheim,[1] olim designationibus 1981 SF2, 1929 WG1, 1949 BU, 1968 DP, 1970 WR, 1977 QJ, 1981 SJ6, et 1981 UB19 agnitus, est asteroides systematis solaris nostri, asteroidibus Cinguli Principalis attributus. Astronomis terrestribus magnitudinem absolutam 13.0 monstrat. Die 26 Septembris 1981 a Normanno G. Thomas, astronomo apud Stationem Anderson Mesa (Observatorium Lowell) versato, repertus est.[2]


Rerum orbitalium ratio epochae 4 Ianuarii 2010 constitit. Qua epocha 3467 Bernheim per dies 1366 circa solem movebatur. Axem orbitalem habebat unitatum astronomicarum 2.41 et eccentricitatem 0.15, distans igitur a sole quam minime unitatibus 2.05, quam maxime unitatibus 2.77. Inclinatio orbitalis 4.11° reperiebatur, anomalia media 124.37°.



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: "2003467" 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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