4786 Tatianina Notae | Nexus externi | Tabula navigationis"Discovery Circumstances: Numbered Minor Planets"2004786Small-Body Database

L +1Latinitas +1 (bona)Asteroides anno 1985 repertiAsteroides Cinguli Principalis


asteroidessystematis solarisasteroidibus Cinguli PrincipalisAstronomismagnitudinem absolutam13 Augusti1985Nicolao Stepanovich ChernykhObservatorium Astrophysicum Crimaeaeepochaeunitatum astronomicarumquam minimequam maximeInclinatio orbitalis°anomalia mediaP literature.svg[1]Small-Body DatabaseMercuriusVenusTellus (Terra)MarsIuppiterSaturnusUranusNeptunusSatellitesLunaAsteroidesindicesCorpora transneptuniana








































4786 Tatianina



Genus

Asteroides Cinguli Principalis
Res orbitales epochae 4 Ianuarii 2010

Excentricitas
0.1919395

Axis semimaior

perihelion
aphelion

2.3585681 UA
1.9058657 UA
2.8112705 UA


Inclinatio orbitalis
7.25246°

Longitudo nodi ascendentis
115.99841°

Argumentum perihelii
117.56242°

Anomalia media
348.09576°

Periodus orbitalis
3.6222700876112 anni
Res physicae

Diameter
— km

Massa

kg

Densitas media
g/cm3

Periodus rotationis

h m

Classis spectralis

Tholen
SMASS



—
Xc


Magnitudo absoluta
13.2

Albedo
—
De recognitione
Primus repertor

N. S. Chernykh
Repertum
die 13 Augusti 1985
Designationes aliae
1985 PE2, 1948 GA, 1970 KF, 1984 EV1, 1984 FM1

4786 Tatianina,[1] olim designationibus 1985 PE2, 1948 GA, 1970 KF, 1984 EV1, et 1984 FM1 agnitus, est asteroides systematis solaris nostri, asteroidibus Cinguli Principalis attributus. Astronomis terrestribus magnitudinem absolutam 13.2 monstrat. Die 13 Augusti 1985 a Nicolao Stepanovich Chernykh, astronomo apud Observatorium Astrophysicum Crimaeae versato, repertus est.[2]


Rerum orbitalium ratio epochae 4 Ianuarii 2010 constitit. Qua epocha 4786 Tatianina per dies 1323 circa solem movebatur. Axem orbitalem habebat unitatum astronomicarum 2.36 et eccentricitatem 0.19, distans igitur a sole quam minime unitatibus 1.91, quam maxime unitatibus 2.81. Inclinatio orbitalis 7.25° reperiebatur, anomalia media 348.1°.



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: "2004786" 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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