3590 Holst Notae | Nexus externi | Tabula navigationis"Discovery Circumstances: Numbered Minor Planets"2003590Small-Body Database

L +1Latinitas +1 (bona)Asteroides anno 1984 repertiAsteroides Cinguli Principalis


asteroidessystematis solarisasteroidibus Cinguli PrincipalisAstronomismagnitudinem absolutam5 Februarii1984Edwardo BowellStationem Anderson Mesa (Observatorium Lowell)epochaeunitatum astronomicarumquam minimequam maximeInclinatio orbitalis°anomalia mediaP literature.svg[1]Small-Body DatabaseMercuriusVenusTellus (Terra)MarsIuppiterSaturnusUranusNeptunusSatellitesLunaAsteroidesindicesCorpora transneptuniana








































3590 Holst



Genus

Asteroides Cinguli Principalis
Res orbitales epochae 4 Ianuarii 2010

Excentricitas
0.0800890

Axis semimaior

perihelion
aphelion

2.2512329 UA
2.0709339 UA
2.4315319 UA


Inclinatio orbitalis
6.70438°

Longitudo nodi ascendentis
128.68746°

Argumentum perihelii
355.07842°

Anomalia media
261.06534°

Periodus orbitalis
3.3778382617385 anni
Res physicae

Diameter

km

Massa

kg

Densitas media
g/cm3

Periodus rotationis

h m

Classis spectralis

Tholen
SMASS



—
—


Magnitudo absoluta
13.1

Albedo
—
De recognitione
Primus repertor

E. Bowell
Repertum
die 5 Februarii 1984
Designationes aliae
1984 CQ, 1954 JC, 1974 FE1

3590 Holst,[1] olim designationibus 1984 CQ, 1954 JC, et 1974 FE1 agnitus, est asteroides systematis solaris nostri, asteroidibus Cinguli Principalis attributus. Astronomis terrestribus magnitudinem absolutam 13.1 monstrat. Die 5 Februarii 1984 ab Edwardo Bowell, astronomo apud Stationem Anderson Mesa (Observatorium Lowell) versato, repertus est.[2]


Rerum orbitalium ratio epochae 4 Ianuarii 2010 constitit. Qua epocha 3590 Holst per dies 1234 circa solem movebatur. Axem orbitalem habebat unitatum astronomicarum 2.25 et eccentricitatem 0.08, distans igitur a sole quam minime unitatibus 2.07, quam maxime unitatibus 2.43. Inclinatio orbitalis 6.7° reperiebatur, anomalia media 261.07°.



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: "2003590" 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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L +1Latinitas +1 (bona)Asteroides anno 1875 repertiAsteroides Cinguli PrincipalisAsteroides a rebus ficticiis appellati Atalaasteroidessystematis solarisasteroidibus Cinguli PrincipalisAstronomismagnitudinem absolutam2 Novembris1875Paulo-Petro HenryObservatorio Lutetiaelitteris Francogallicis1801Castrobrientiiepochaeunitatum astronomicarumquam minimequam maximeInclinatio orbitalis°anomalia media [1]Small-Body DatabaseMercuriusVenusTellus (Terra)MarsIuppiterSaturnusUranusNeptunusSatellitesLunaAsteroidesindicesCorpora transneptuniana Vide etiam paginam discretivam: Atala 152 Atala Genus Asteroides Cinguli Principalis Res orbitales epochae 4 Ianuarii 2010 Excentricitas 0.0754396 Axis semimaior perihelion aphelion 3.1399791 UA 2.9031003 UA 3.3768579 UA Inclinatio orbitalis 12.11235° Longitudo nodi ascendentis 40.00824° Argumentum perihelii 58.52961° Anomalia media 348.89681° Periodus orbitalis 5.5641436375086 anni Res physicae Diameter km Massa kg Densitas media g/cm 3 Periodus rotation
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