135 Hertha Notae | Nexus externi | Tabula navigationis"Discovery Circumstances: Numbered Minor Planets"2000135Small-Body Database

L +1Latinitas +1 (bona)Asteroides anno 1874 repertiAsteroides Cinguli PrincipalisAsteroides praenominibus appellati


asteroidessystematis solarisasteroidibus Cinguli PrincipalisAstronomismagnitudinem absolutam18 Februarii1874Christiano Henrico Friderico PetersObservatorio LitchfieldGermanicumGermaniciNerthiTacitoepochaeunitatum astronomicarumquam minimequam maximeInclinatio orbitalis°anomalia mediaP literature.svg[1]Small-Body DatabaseMercuriusVenusTellus (Terra)MarsIuppiterSaturnusUranusNeptunusSatellitesLunaAsteroidesindicesCorpora transneptuniana





Vide etiam paginam fere homonymam: Hertha (praenomen)





































135 Hertha



Genus

Asteroides Cinguli Principalis
Res orbitales epochae 4 Ianuarii 2010

Excentricitas
.2058381644573652

Axis semimaior

perihelion
aphelion

2.429387379296731 UA
1.929326740386403 UA
2.929448018207059 UA


Inclinatio orbitalis
2.305062267489665°

Longitudo nodi ascendentis
343.8396033333133°

Argumentum perihelii
340.0404730744327°

Anomalia media
172.5423588525037°

Periodus orbitalis
3.7866342499438 anni
Res physicae

Diameter

km

Massa

kg

Densitas media
g/cm3

Periodus rotationis
8 h 24.036026 m

Classis spectralis

Tholen
SMASS



M
Xk


Magnitudo absoluta
8.23

Albedo
0.1436
De recognitione
Primus repertor

C. H. F. Peters
Repertum
die 18 Februarii 1874
Designationes aliae

135 Hertha[1] est asteroides systematis solaris nostri, asteroidibus Cinguli Principalis attributus. Astronomis terrestribus magnitudinem absolutam 8.23 monstrat. Die 18 Februarii 1874 a Christiano Henrico Friderico Peters in Observatorio Litchfield versato repertus est.[2]Hertha, e qua asteroides appellatus est, est praenomen femininum Germanicum ex errore orthographico, ut censetur, ortum; nomen enim dei Germanici Nerthi, a Tacito tradita, olim littera H loco N lectum est.[3]


Rerum orbitalium ratio epochae 4 Ianuarii 2010 constitit. Qua epocha 135 Hertha per dies 1383 circa solem movebatur. Axem orbitalem habebat unitatum astronomicarum 2.43 et eccentricitatem 0.21, distans igitur a sole quam minime unitatibus 1.93, quam maxime unitatibus 2.93. Inclinatio orbitalis 2.31° reperiebatur, anomalia media 172.54°.



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 


  3. ↑ Sic de:Hertha



Nexus externi |





Wikidata-logo.svg
Data astronomica: "2000135" 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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