Eris (planetula) - la.LinkFang.org

Eris (planetula)




Eris
Inventio
Inventus a M. E. Brown, C. Trujillo; D. Rabinowitz
Inventus anno 2003
Proprietates orbitales
Axis semimaior > 30 ua
Radius 1163 km
Perihelion ca. 34 ua
Aphelion ca. 98 ua
Eccentricitas ...
Periodus orbitalis 557 a
Inclinatio orbitalis ..°
Satellites 1
Satellitum nomina Dysnomia
Proprietates physicales
Diametrus 2.325 km
Area .. km2
Massa 1,3×1022 kg
Densitas 2,3 g/cm3
Gravitas 0,6 m/s2
Velocitas fugiendi km/s
Periodus rotationis ? d
Inclinatio axialis ..
Albedo ?
Temperatura
min med max
- K 34 K - K
Proprietates atmosphericae
Pressio atmosphaerica kPa
Carbonium %
Nitrogenium %

(136199) Eris (-idis, f.; primum 2003 UB313 nominata) est planetula, cuius diametrus est circiter 2325 km. Inde magnitudine aequat Plutoni, sed pondere maius obiectum zonae Kuiperi videtur. Diametrum satis compertum habemus, postquam Eris ante stellam remotam migrans eius lucem obscuravit (mense Oct. 2010). Eris inventa est mense Octobri 2003, sed e photographemate data tunc incerta erant. Mense autem Decembri 2004 nova data inventionem certam fecere. Magnitudine Eridis astronomi coacti sunt, ut definitionem planetarum denuo cogitarent et novum genus planetularum instituerent. Inde Eris in numero planetularum habetur sicut Pluto.

Mense Septembri 2005 parva satelles inventa est quae circum Eridem orbita 14 dierum revolvitur et Dysnomia appellatur.


Systema Solare nostrum
Sol

Planetae: Mercurius | Venus | Tellus (Terra) | Mars | Iuppiter | Saturnus | Uranus | Neptunus

Planetulae: Ceres | Pluto | Haumea | Makemake | Eris | 225088 (2007 OR10)

Corpora alia: Satellites | Luna | Asteroides (+ indices) | Corpora transneptuniana

Vide etiam indices corporum Systematis Solaris redactos secundum radium et massam.





Categoriae: Planetulae Systematis Solaris | Corpora Ultraneptuniana



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