7797 Morita Notae | Nexus externi | Tabula navigationis"Discovery Circumstances: Numbered Minor Planets"2007797Small-Body Database

L +1Latinitas +1 (bona)Asteroides anno 1996 repertiAsteroides Cinguli Principalis


asteroidessystematis solarisasteroidibus Cinguli PrincipalisAstronomismagnitudinem absolutam26 Ianuarii1996Takao KobayashiObservatorium Ōizumiepochaeunitatum astronomicarumquam minimequam maximeInclinatio orbitalis°anomalia mediaP literature.svg[1]Small-Body DatabaseMercuriusVenusTellus (Terra)MarsIuppiterSaturnusUranusNeptunusSatellitesLunaAsteroidesindicesCorpora transneptuniana








































7797 Morita



Genus

Asteroides Cinguli Principalis
Res orbitales epochae 4 Ianuarii 2010

Excentricitas
0.1476714

Axis semimaior

perihelion
aphelion

3.1841529 UA
2.7139446 UA
3.6543612 UA


Inclinatio orbitalis
12.95681°

Longitudo nodi ascendentis
152.84213°

Argumentum perihelii
202.96804°

Anomalia media
284.57317°

Periodus orbitalis
5.6819719939767 anni
Res physicae

Diameter
— km

Massa

kg

Densitas media
g/cm3

Periodus rotationis

h m

Classis spectralis

Tholen
SMASS



—
—


Magnitudo absoluta
11.3

Albedo
—
De recognitione
Primus repertor

T. Kobayashi
Repertum
die 26 Ianuarii 1996
Designationes aliae
1996 BK2, 1953 QQ, 1962 CM, 1982 TA3, 1985 DG4, 1991 EA6

7797 Morita,[1] olim designationibus 1996 BK2, 1953 QQ, 1962 CM, 1982 TA3, 1985 DG4, et 1991 EA6 agnitus, est asteroides systematis solaris nostri, asteroidibus Cinguli Principalis attributus. Astronomis terrestribus magnitudinem absolutam 11.3 monstrat. Die 26 Ianuarii 1996 a Takao Kobayashi, astronomo apud Observatorium Ōizumi versato, repertus est.[2]


Rerum orbitalium ratio epochae 4 Ianuarii 2010 constitit. Qua epocha 7797 Morita per dies 2075 circa solem movebatur. Axem orbitalem habebat unitatum astronomicarum 3.18 et eccentricitatem 0.15, distans igitur a sole quam minime unitatibus 2.71, quam maxime unitatibus 3.65. Inclinatio orbitalis 12.96° reperiebatur, anomalia media 284.57°.



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: "2007797" 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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