4070 Rozov Notae | Nexus externi | Tabula navigationis"Discovery Circumstances: Numbered Minor Planets"2004070Small-Body Database

L +1Latinitas +1 (bona)Asteroides anno 1980 repertiAsteroides Cinguli Principalis


asteroidessystematis solarisasteroidibus Cinguli PrincipalisAstronomismagnitudinem absolutam8 Septembris1980Ludmila ŽuravlëvaObservatorium Astrophysicum Crimaeaeepochaeunitatum astronomicarumquam minimequam maximeInclinatio orbitalis°anomalia mediaP literature.svg[1]Small-Body DatabaseMercuriusVenusTellus (Terra)MarsIuppiterSaturnusUranusNeptunusSatellitesLunaAsteroidesindicesCorpora transneptuniana








































4070 Rozov



Genus

Asteroides Cinguli Principalis
Res orbitales epochae 4 Ianuarii 2010

Excentricitas
0.1673113

Axis semimaior

perihelion
aphelion

2.2507048 UA
1.8741365 UA
2.6272731 UA


Inclinatio orbitalis
3.78229°

Longitudo nodi ascendentis
253.33806°

Argumentum perihelii
123.84652°

Anomalia media
230.98951°

Periodus orbitalis
3.3766496900753 anni
Res physicae

Diameter
— km

Massa

kg

Densitas media
g/cm3

Periodus rotationis

h m

Classis spectralis

Tholen
SMASS



—
—


Magnitudo absoluta
13.3

Albedo
—
De recognitione
Primus repertor

L. Žuravlëva
Repertum
die 8 Septembris 1980
Designationes aliae
1980 RS2, 1953 TX, 1953 VO

4070 Rozov,[1] olim designationibus 1980 RS2, 1953 TX, et 1953 VO agnitus, est asteroides systematis solaris nostri, asteroidibus Cinguli Principalis attributus. Astronomis terrestribus magnitudinem absolutam 13.3 monstrat. Die 8 Septembris 1980 a Ludmila Žuravlëva, astronomo apud Observatorium Astrophysicum Crimaeae versato, repertus est.[2]


Rerum orbitalium ratio epochae 4 Ianuarii 2010 constitit. Qua epocha 4070 Rozov per dies 1233 circa solem movebatur. Axem orbitalem habebat unitatum astronomicarum 2.25 et eccentricitatem 0.17, distans igitur a sole quam minime unitatibus 1.87, quam maxime unitatibus 2.63. Inclinatio orbitalis 3.78° reperiebatur, anomalia media 230.99°.



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: "2004070" 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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