4570 Runcorn Notae | Nexus externi | Tabula navigationis"Discovery Circumstances: Numbered Minor Planets"2004570Small-Body Database

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


asteroidessystematis solarisasteroidibus Cinguli PrincipalisAstronomismagnitudinem absolutam14 Augusti1985Edwardo BowellObservatorium Lowell (Statio Anderson Mesa)epochaeunitatum astronomicarumquam minimequam maximeInclinatio orbitalis°anomalia mediaP literature.svg[1]Small-Body DatabaseMercuriusVenusTellus (Terra)MarsIuppiterSaturnusUranusNeptunusSatellitesLunaAsteroidesindicesCorpora transneptuniana








































4570 Runcorn



Genus

Asteroides Cinguli Principalis
Res orbitales epochae 4 Ianuarii 2010

Excentricitas
0.1095657

Axis semimaior

perihelion
aphelion

2.1983493 UA
1.9574856 UA
2.4392130 UA


Inclinatio orbitalis
5.01975°

Longitudo nodi ascendentis
349.32284°

Argumentum perihelii
208.54705°

Anomalia media
296.74037°

Periodus orbitalis
3.259517127447 anni
Res physicae

Diameter
— km

Massa

kg

Densitas media
g/cm3

Periodus rotationis

h m

Classis spectralis

Tholen
SMASS



—
Sa


Magnitudo absoluta
13.0

Albedo
—
De recognitione
Primus repertor

E. Bowell
Repertum
die 14 Augusti 1985
Designationes aliae
1985 PR, 1969 TO, 1971 BU1, 1982 SB11, 1984 DY1, 1985 RF4, 1986 XC3

4570 Runcorn,[1] olim designationibus 1985 PR, 1969 TO, 1971 BU1, 1982 SB11, 1984 DY1, 1985 RF4, et 1986 XC3 agnitus, est asteroides systematis solaris nostri, asteroidibus Cinguli Principalis attributus. Astronomis terrestribus magnitudinem absolutam 13.0 monstrat. Die 14 Augusti 1985 ab Edwardo Bowell, astronomo apud Observatorium Lowell (Statio Anderson Mesa) versato, repertus est.[2]


Rerum orbitalium ratio epochae 4 Ianuarii 2010 constitit. Qua epocha 4570 Runcorn per dies 1191 circa solem movebatur. Axem orbitalem habebat unitatum astronomicarum 2.2 et eccentricitatem 0.11, distans igitur a sole quam minime unitatibus 1.96, quam maxime unitatibus 2.44. Inclinatio orbitalis 5.02° reperiebatur, anomalia media 296.74°.



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: "2004570" 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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