8053 Kleist Notae | Nexus externi | Tabula navigationis"Discovery Circumstances: Numbered Minor Planets"2008053Small-Body Database

L +1Latinitas +1 (bona)Asteroides anno 1960 repertiAsteroides Cinguli Principalis


asteroidessystematis solarisasteroidibus Cinguli PrincipalisAstronomismagnitudinem absolutam25 Septembris1960Cornelio Ioanne van HoutenIngrid Mortimer van Houten-GroeneveldThoma GehrelsObservatorium Palomarepochaeunitatum astronomicarumquam minimequam maximeInclinatio orbitalis°anomalia mediaP literature.svg[1]Small-Body DatabaseMercuriusVenusTellus (Terra)MarsIuppiterSaturnusUranusNeptunusSatellitesLunaAsteroidesindicesCorpora transneptuniana








































8053 Kleist



Genus

Asteroides Cinguli Principalis
Res orbitales epochae 4 Ianuarii 2010

Excentricitas
0.1627312

Axis semimaior

perihelion
aphelion

2.3850409 UA
1.9969203 UA
2.7731615 UA


Inclinatio orbitalis
1.57277°

Longitudo nodi ascendentis
323.06463°

Argumentum perihelii
261.77769°

Anomalia media
266.15443°

Periodus orbitalis
3.6834260574949 anni
Res physicae

Diameter
— km

Massa

kg

Densitas media
g/cm3

Periodus rotationis

h m

Classis spectralis

Tholen
SMASS



—
—


Magnitudo absoluta
14.0

Albedo
—
De recognitione
Primi repertores

C. I. van Houten, I. M. van Houten-Groeneveld, T. Gehrels
Repertum
die 25 Septembris 1960
Designationes aliae
4082 P-L, 1992 EV, 1993 RP9

8053 Kleist,[1] olim designationibus 4082 P-L, 1992 EV, et 1993 RP9 agnitus, est asteroides systematis solaris nostri, asteroidibus Cinguli Principalis attributus. Astronomis terrestribus magnitudinem absolutam 14.0 monstrat. Die 25 Septembris 1960 a Cornelio Ioanne van Houten, Ingrid Mortimer van Houten-Groeneveld, et Thoma Gehrels, astronomis apud Observatorium Palomar versatis, repertus est.[2]


Rerum orbitalium ratio epochae 4 Ianuarii 2010 constitit. Qua epocha 8053 Kleist per dies 1345 circa solem movebatur. Axem orbitalem habebat unitatum astronomicarum 2.39 et eccentricitatem 0.16, distans igitur a sole quam minime unitatibus 2, quam maxime unitatibus 2.77. Inclinatio orbitalis 1.57° reperiebatur, anomalia media 266.15°.



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: "2008053" 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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