8819 Chrisbondi Notae | Nexus externi | Tabula navigationis"Discovery Circumstances: Numbered Minor Planets"2008819Small-Body Database

L +1Latinitas +1 (bona)Asteroides anno 1985 repertiAsteroides Cinguli Principalis


asteroidessystematis solarisasteroidibus Cinguli PrincipalisAstronomismagnitudinem absolutam14 Septembris1985Henrico DebehogneObservatorium Europaeum Australiepochaeunitatum astronomicarumquam minimequam maximeInclinatio orbitalis°anomalia mediaP literature.svg[1]Small-Body DatabaseMercuriusVenusTellus (Terra)MarsIuppiterSaturnusUranusNeptunusSatellitesLunaAsteroidesindicesCorpora transneptuniana








































8819 Chrisbondi



Genus

Asteroides Cinguli Principalis
Res orbitales epochae 4 Ianuarii 2010

Excentricitas
0.1690261

Axis semimaior

perihelion
aphelion

2.7818814 UA
2.3116708 UA
3.2520920 UA


Inclinatio orbitalis
9.38590°

Longitudo nodi ascendentis
179.44399°

Argumentum perihelii
157.84899°

Anomalia media
96.32007°

Periodus orbitalis
4.6399802888433 anni
Res physicae

Diameter
— km

Massa

kg

Densitas media
g/cm3

Periodus rotationis

h m

Classis spectralis

Tholen
SMASS



—
—


Magnitudo absoluta
13.5

Albedo
—
De recognitione
Primus repertor

H. Debehogne
Repertum
die 14 Septembris 1985
Designationes aliae
1985 RR4, 1990 UD4

8819 Chrisbondi,[1] olim designationibus 1985 RR4 et 1990 UD4 agnitus, est asteroides systematis solaris nostri, asteroidibus Cinguli Principalis attributus. Astronomis terrestribus magnitudinem absolutam 13.5 monstrat. Die 14 Septembris 1985 ab Henrico Debehogne, astronomo apud Observatorium Europaeum Australi versato, repertus est.[2]


Rerum orbitalium ratio epochae 4 Ianuarii 2010 constitit. Qua epocha 8819 Chrisbondi per dies 1695 circa solem movebatur. Axem orbitalem habebat unitatum astronomicarum 2.78 et eccentricitatem 0.17, distans igitur a sole quam minime unitatibus 2.31, quam maxime unitatibus 3.25. Inclinatio orbitalis 9.39° reperiebatur, anomalia media 96.32°.



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: "2008819" 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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