4087 Pärt Notae | Nexus externi | Tabula navigationis"Discovery Circumstances: Numbered Minor Planets"2004087Small-Body Database

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


asteroidessystematis solarisasteroidibus Cinguli PrincipalisAstronomismagnitudinem absolutam5 Martii1986Edwardo BowellObservatorium Lowellepochaeunitatum astronomicarumquam minimequam maximeInclinatio orbitalis°anomalia mediaP literature.svg[1]Small-Body DatabaseMercuriusVenusTellus (Terra)MarsIuppiterSaturnusUranusNeptunusSatellitesLunaAsteroidesindicesCorpora transneptuniana








































4087 Pärt



Genus

Asteroides Cinguli Principalis
Res orbitales epochae 4 Ianuarii 2010

Excentricitas
0.1179718

Axis semimaior

perihelion
aphelion

2.1767921 UA
1.9199920 UA
2.4335922 UA


Inclinatio orbitalis
4.42557°

Longitudo nodi ascendentis
24.77388°

Argumentum perihelii
303.64807°

Anomalia media
18.06187°

Periodus orbitalis
3.2116900687201 anni
Res physicae

Diameter
— km

Massa

kg

Densitas media
g/cm3

Periodus rotationis
16 h 28.199959 m

Classis spectralis

Tholen
SMASS



—
—


Magnitudo absoluta
13.3

Albedo
—
De recognitione
Primus repertor

E. Bowell
Repertum
die 5 Martii 1986
Designationes aliae
1986 EM1, 1951 KV, 1970 GT, 1974 TT, 1974 UP, 1983 JT

4087 Pärt,[1] olim designationibus 1986 EM1, 1951 KV, 1970 GT, 1974 TT, 1974 UP, et 1983 JT agnitus, est asteroides systematis solaris nostri, asteroidibus Cinguli Principalis attributus. Astronomis terrestribus magnitudinem absolutam 13.3 monstrat. Die 5 Martii 1986 ab Edwardo Bowell, astronomo apud Observatorium Lowell versato, repertus est.[2]


Rerum orbitalium ratio epochae 4 Ianuarii 2010 constitit. Qua epocha 4087 Pärt per dies 1173 circa solem movebatur. Axem orbitalem habebat unitatum astronomicarum 2.18 et eccentricitatem 0.12, distans igitur a sole quam minime unitatibus 1.92, quam maxime unitatibus 2.43. Inclinatio orbitalis 4.43° reperiebatur, anomalia media 18.06°.



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: "2004087" 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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