4022 Nonna Notae | Nexus externi | Tabula navigationis"Discovery Circumstances: Numbered Minor Planets"2004022Small-Body Database

L +1Latinitas +1 (bona)Asteroides anno 1981 repertiAsteroides Cinguli Principalis


asteroidessystematis solarisasteroidibus Cinguli PrincipalisAstronomismagnitudinem absolutam8 Octobris1981Lyudmila Ivanovna ChernykhObservatorium Astrophysicum Crimaeaeepochaeunitatum astronomicarumquam minimequam maximeInclinatio orbitalis°anomalia mediaP literature.svg[1]Small-Body DatabaseMercuriusVenusTellus (Terra)MarsIuppiterSaturnusUranusNeptunusSatellitesLunaAsteroidesindicesCorpora transneptuniana








































4022 Nonna



Genus

Asteroides Cinguli Principalis
Res orbitales epochae 4 Ianuarii 2010

Excentricitas
0.1285135

Axis semimaior

perihelion
aphelion

2.3579705 UA
2.0549395 UA
2.6610015 UA


Inclinatio orbitalis
5.09735°

Longitudo nodi ascendentis
278.51768°

Argumentum perihelii
33.77593°

Anomalia media
3.10001°

Periodus orbitalis
3.6208934652977 anni
Res physicae

Diameter
— km

Massa

kg

Densitas media
g/cm3

Periodus rotationis

h m

Classis spectralis

Tholen
SMASS



—
—


Magnitudo absoluta
12.7

Albedo
—
De recognitione
Primus repertor

L. I. Chernykh
Repertum
die 8 Octobris 1981
Designationes aliae
1981 TL4, 1966 PC, 1984 OJ

4022 Nonna,[1] olim designationibus 1981 TL4, 1966 PC, et 1984 OJ agnitus, est asteroides systematis solaris nostri, asteroidibus Cinguli Principalis attributus. Astronomis terrestribus magnitudinem absolutam 12.7 monstrat. Die 8 Octobris 1981 a Lyudmila Ivanovna Chernykh, astronomo apud Observatorium Astrophysicum Crimaeae versato, repertus est.[2]


Rerum orbitalium ratio epochae 4 Ianuarii 2010 constitit. Qua epocha 4022 Nonna per dies 1323 circa solem movebatur. Axem orbitalem habebat unitatum astronomicarum 2.36 et eccentricitatem 0.13, distans igitur a sole quam minime unitatibus 2.05, quam maxime unitatibus 2.66. Inclinatio orbitalis 5.1° reperiebatur, anomalia media 3.1°.



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: "2004022" 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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