78 Diana Notae | Nexus externi | Tabula navigationis"Discovery Circumstances: Numbered Minor Planets"2000078Small-Body Database

L +1Latinitas +1 (bona)Asteroides anno 1863 repertiAsteroides Cinguli PrincipalisAsteroides e mythologia Romana appellati


Diana (discretiva)asteroidessystematis solarisasteroidibus Cinguli PrincipalisAstronomismagnitudinem absolutam15 Martii1863Carolo Theodoro Roberto LutherDusseldorpioDianamythologia RomanadeaArtemidideae Graecaeepochaeunitatum astronomicarumquam minimequam maximeInclinatio orbitalis°anomalia mediaP literature.svg[1]Small-Body DatabaseMercuriusVenusTellus (Terra)MarsIuppiterSaturnusUranusNeptunusSatellitesLunaAsteroidesindicesCorpora transneptuniana





Vide etiam paginam discretivam: Diana (discretiva)







































78 Diana



Genus

Asteroides Cinguli Principalis
Res orbitales epochae 4 Ianuarii 2010

Excentricitas
.206440776441907

Axis semimaior

perihelion
aphelion

2.621552007429455 UA
2.080356775532878 UA
3.162747239326032 UA


Inclinatio orbitalis
8.704882670391418°

Longitudo nodi ascendentis
333.4589117192108°

Argumentum perihelii
152.6086634526031°

Anomalia media
247.8726898087476°

Periodus orbitalis
4.2446894221408 anni
Res physicae

Diameter

km

Massa

kg

Densitas media
g/cm3

Periodus rotationis
7 h 13.499994 m

Classis spectralis

Tholen
SMASS



C
Ch


Magnitudo absoluta
8.09

Albedo
0.0706
De recognitione
Primus repertor

K. Luther
Repertum
die 15 Martii 1863
Designationes aliae

78 Diana[1] est asteroides systematis solaris nostri, asteroidibus Cinguli Principalis attributus. Astronomis terrestribus magnitudinem absolutam 8.09 monstrat. Die 15 Martii 1863 a Carolo Theodoro Roberto Luther in Dusseldorpio versato repertus est.[2]Diana, e qua asteroides appellatur, in mythologia Romana fuit dea venationis, Artemidi deae Graecae respondens.


Rerum orbitalium ratio epochae 4 Ianuarii 2010 constitit. Qua epocha 78 Diana per dies 1550 circa solem movebatur. Axem orbitalem habebat unitatum astronomicarum 2.62 et eccentricitatem 0.21, distans igitur a sole quam minime unitatibus 2.08, quam maxime unitatibus 3.16. Inclinatio orbitalis 8.7° reperiebatur, anomalia media 247.87°.



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: "2000078" 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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