35 Leukothea Notae | Nexus externi | Tabula navigationis"Discovery Circumstances: Numbered Minor Planets"2000035Small-Body Database

L +1Latinitas +1 (bona)Asteroides anno 1855 repertiAsteroides Cinguli PrincipalisAsteroides e mythologia Graeca appellati


Leucothea (discretiva)asteroidessystematis solarisasteroidibus Cinguli PrincipalisAstronomismagnitudinem absolutam19 Aprilis1855Carolo Theodoro Roberto LutherDusseldorpiomythologia GraecaLeucotheaSemelesDionysiepochaeunitatum astronomicarumquam minimequam maximeInclinatio orbitalis°anomalia mediaP literature.svg[1]Small-Body DatabaseMercuriusVenusTellus (Terra)MarsIuppiterSaturnusUranusNeptunusSatellitesLunaAsteroidesindicesCorpora transneptuniana





Vide etiam paginam discretivam: Leucothea (discretiva)







































35 Leukothea



Genus

Asteroides Cinguli Principalis
Res orbitales epochae 4 Ianuarii 2010

Excentricitas
0.2275131

Axis semimaior

perihelion
aphelion

2.9919498 UA
2.3112420 UA
3.6726576 UA


Inclinatio orbitalis
7.93483°

Longitudo nodi ascendentis
353.80087°

Argumentum perihelii
213.87737°

Anomalia media
287.24602°

Periodus orbitalis
5.1753490425736 anni
Res physicae

Diameter

km

Massa

kg

Densitas media
g/cm3

Periodus rotationis
32 h 0.0 m

Classis spectralis

Tholen
SMASS



C
C


Magnitudo absoluta
8.50

Albedo
0.0662
De recognitione
Primus repertor

K. Luther
Repertum
die 19 Aprilis 1855
Designationes aliae
1948 DC, 1950 RS1, 1976 WH

35 Leukothea,[1] olim designationibus 1948 DC, 1950 RS1, et 1976 WH agnitus, est asteroides systematis solaris nostri, asteroidibus Cinguli Principalis attributus. Astronomis terrestribus magnitudinem absolutam 8.50 monstrat. Die 19 Aprilis 1855 a Carolo Theodoro Roberto Luther in Dusseldorpio versato repertus est.[2] In mythologia Graeca Leucothea, e qua asteroides appellatus est, fuit dea marina quae olim nomen mortale "Ino" gerebat, soror Semeles, Dionysi infantis protectrix.


Rerum orbitalium ratio epochae 4 Ianuarii 2010 constitit. Qua epocha 35 Leukothea per dies 1890 circa solem movebatur. Axem orbitalem habebat unitatum astronomicarum 2.99 et eccentricitatem 0.23, distans igitur a sole quam minime unitatibus 2.31, quam maxime unitatibus 3.67. Inclinatio orbitalis 7.93° reperiebatur, anomalia media 287.25°.





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: "2000035" 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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