4090 Říšehvězd Notae | Nexus externi | Tabula navigationis"Discovery Circumstances: Numbered Minor Planets"2004090Small-Body Database

L +1Latinitas +1 (bona)Asteroides anno 1986 repertiAsteroides Cinguli Principalis


asteroidessystematis solarisasteroidibus Cinguli PrincipalisAstronomismagnitudinem absolutam2 Septembris1986Antonio MrkosObservatorium Kleťepochaeunitatum astronomicarumquam minimequam maximeInclinatio orbitalis°anomalia mediaP literature.svg[1]Small-Body DatabaseMercuriusVenusTellus (Terra)MarsIuppiterSaturnusUranusNeptunusSatellitesLunaAsteroidesindicesCorpora transneptuniana








































4090 Říšehvězd



Genus

Asteroides Cinguli Principalis
Res orbitales epochae 4 Ianuarii 2010

Excentricitas
0.2087417

Axis semimaior

perihelion
aphelion

2.3579286 UA
1.8657306 UA
2.8501266 UA


Inclinatio orbitalis
1.32573°

Longitudo nodi ascendentis
266.69897°

Argumentum perihelii
3.60426°

Anomalia media
211.64575°

Periodus orbitalis
3.6207970277892 anni
Res physicae

Diameter
— km

Massa

kg

Densitas media
g/cm3

Periodus rotationis

h m

Classis spectralis

Tholen
SMASS






Magnitudo absoluta
13.4

Albedo

De recognitione
Primus repertor

A. Mrkos
Repertum
die 2 Septembris 1986
Designationes aliae
1986 RH1, 1931 FF, 1971 KB, 1982 KX, 1988 AR3, 1989 GU

4090 Říšehvězd,[1] olim designationibus 1986 RH1, 1931 FF, 1971 KB, 1982 KX, 1988 AR3, et 1989 GU agnitus, est asteroides systematis solaris nostri, asteroidibus Cinguli Principalis attributus. Astronomis terrestribus magnitudinem absolutam 13.4 monstrat. Die 2 Septembris 1986 ab Antonio Mrkos, astronomo apud Observatorium Kleť versato, repertus est.[2]


Rerum orbitalium ratio epochae 4 Ianuarii 2010 constitit. Qua epocha 4090 Říšehvězd per dies 1322 circa solem movebatur. Axem orbitalem habebat unitatum astronomicarum 2.36 et eccentricitatem 0.21, distans igitur a sole quam minime unitatibus 1.87, quam maxime unitatibus 2.85. Inclinatio orbitalis 1.33° reperiebatur, anomalia media 211.65°.



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: "2004090" 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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