1790 Volkov Notae | Nexus externi | Tabula navigationis"Discovery Circumstances: Numbered Minor Planets"2001790Small-Body Database

L +1Latinitas +1 (bona)Asteroides anno 1967 repertiAsteroides Cinguli Principalis


asteroidessystematis solarisasteroidibus Cinguli PrincipalisAstronomismagnitudinem absolutam9 Martii1967Lyudmila Ivanovna ChernykhObservatorio Astrophysico Crimaeaeepochaeunitatum astronomicarumquam minimequam maximeInclinatio orbitalis°anomalia mediaP literature.svg[1]Small-Body DatabaseMercuriusVenusTellus (Terra)MarsIuppiterSaturnusUranusNeptunusSatellitesLunaAsteroidesindicesCorpora transneptuniana








































1790 Volkov



Genus

Asteroides Cinguli Principalis
Res orbitales epochae 4 Ianuarii 2010

Excentricitas
0.1011056

Axis semimaior

perihelion
aphelion

2.2377719 UA
2.0115206 UA
2.4640232 UA


Inclinatio orbitalis
5.11294°

Longitudo nodi ascendentis
2.07868°

Argumentum perihelii
147.94832°

Anomalia media
300.99258°

Periodus orbitalis
3.3475873147159 anni
Res physicae

Diameter

km

Massa

kg

Densitas media
g/cm3

Periodus rotationis

h m

Classis spectralis

Tholen
SMASS






Magnitudo absoluta
12.5

Albedo

De recognitione
Primus repertor

L. I. Chernykh
Repertum
die 9 Martii 1967
Designationes aliae
1967 ER, 1926 AB, 1950 BU1, 1955 SV2, 1957 FB

1790 Volkov,[1] olim designationibus 1967 ER, 1926 AB, 1950 BU1, 1955 SV2, et 1957 FB agnitus, est asteroides systematis solaris nostri, asteroidibus Cinguli Principalis attributus. Astronomis terrestribus magnitudinem absolutam 12.5 monstrat. Die 9 Martii 1967 a Lyudmila Ivanovna Chernykh in Observatorio Astrophysico Crimaeae versato repertus est.[2]


Rerum orbitalium ratio epochae 4 Ianuarii 2010 constitit. Qua epocha 1790 Volkov per dies 1223 circa solem movebatur. Axem orbitalem habebat unitatum astronomicarum 2.24 et eccentricitatem 0.1, distans igitur a sole quam minime unitatibus 2.01, quam maxime unitatibus 2.46. Inclinatio orbitalis 5.11° reperiebatur, anomalia media 300.99°.



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: "2001790" 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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