Eris
![]() Eris, aur iske chaand, Dysnomia ke low-resolution chhaapa, jiske Hubble Space Telescope, August 2006 me utaris rahaa | |||||||||
Discovery | |||||||||
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Discovered by | |||||||||
Discovery date | January 5, 2005 | ||||||||
Designations | |||||||||
(136199) Eris | |||||||||
Pronunciation | /ˈɛrɪs/,[1] /ˈɪərɪs/[2]</ref> | ||||||||
Named after | Ἔρις Eris | ||||||||
Template:Mp Xena (nickname) | |||||||||
Adjectives | Eridian /ɛˈrɪdiən/[3] | ||||||||
Symbol | ![]() | ||||||||
Orbital characteristics | |||||||||
Epoch May 5, 2025 (JD 2460800.5) | |||||||||
Earliest precovery date | September 3, 1954 | ||||||||
Aphelion | 97.699 AU (14.616×10 9 km) | ||||||||
Perihelion | 38.403 AU (5.745×10 9 km) | ||||||||
68.051 AU (10.180 Tm) | |||||||||
Eccentricity | 0.43568 | ||||||||
561.38 yr (205,044 d) | |||||||||
Average orbital speed | 3.434 km/s | ||||||||
211.032° | |||||||||
Template:Deg2DMS / day | |||||||||
Inclination | 43.822° | ||||||||
36.046° | |||||||||
≈ December 7, 2257 | |||||||||
150.714° | |||||||||
Known satellites | 1 (Dysnomia) | ||||||||
Physical characteristics | |||||||||
2326±12 km | |||||||||
1163±6 km | |||||||||
(1.70±0.02)×107 km2 | |||||||||
Volume | (6.59±0.10)×109 km3 | ||||||||
Mass | |||||||||
Mean density | 2.43±0.05 g/cm3 | ||||||||
Equatorial surface gravity | 0.82±0.02 m/s2 0.084±0.002 g | ||||||||
Equatorial escape velocity | Template:V2 ± 0.01 km/s | ||||||||
15.786 d (synchronous) | |||||||||
≈ 78.3° to orbit (assumed) ≈ 61.6° to ecliptic (assumed) = 28.41° for the north pole of Dysnomia's orbit, | |||||||||
0.96+0.09 −0.04 Template:Sic geometric 0.99+0.01 −0.09 Bond | |||||||||
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B−V=0.78, V−R=0.45[5] | |||||||||
18.7 | |||||||||
–1.21 | |||||||||
34.4±1.4 milli-arcsec |
Eris (minor-planet designation: 136199 Eris), sab se jaada garrhu aur duusra sab se barraa bauna grah, Saur Mandal me hae. [6] Ii ek trans-Neptunian object (TNO) hae aur iske high-eccentricity orbit hae. Eris ke January 2005 me Palomar Observatory–based team, jike Mike Brown lead karis rahaa, paaais rahaa aur iske ek saal baad fir se verify karaa gais rahaa. Iska naam September 2006 me, GrecoTemplate:En dashRoman deota ke baad rakkhaa gais rahaa. Suraj ke parikrama kare waala chij me se, Eris 9th sab se garrhu hae, aur agar sab chaand ke lewa jaae tan ii 16th hae. Ii saur mandal ke sab se barraa chij hae jiske koi spacecraft visit nai karis hae. Eris ke diameter 2,326 ± 12 kilometres (1,445 ± 7 mi) hae; iske wajan dunia ke 0.28% hae aur Yamgrah se 27% jaada hae, jabki Yamgrah, by volume, thorraa barraa hae. Duuno Eris aur Yamgrah kesurface area Russia nai to South America ke baraabar hae.
Saur mandal (Solar System)
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Suraj • Heliosphere |
Grah (Planets) ☾ = Chaand ∅ = rings |
Budhgrah (Mercury) | Sukhgrah (Venus) | Dunia (Earth) ☾ | Mangalgrah (Mars) ☾ | ||
Brahaspati (Jupiter) ☾ ∅ | Sanigrah (Saturn) ☾ ∅ | Arungrah (Uranus) ☾ ∅ | Varungrah (Neptune) ☾ ∅ | ||||
Bauna grah (Dwarf planet) |
Ceres | Pluto ☾ | Haumea ☾ | Makemake | |||
Eris ☾ | |||||||
Small Solar System bodies |
Chhota tara (Asteroid) (minor planets) |
Groups and families: Vulcanoids · Near-Earth asteroids · Asteroid belt Jupiter Trojans · Centaurs · Neptune Trojans · Asteroid moons · Meteoroids · Pallas · Juno · Vesta · Hygiea · | |||||
See also the list of asteroids. | |||||||
Trans- Neptunians |
Kuiper belt – Plutinos: Orcus · Ixion – Cubewanos: Varuna · Quaoar · Huya | ||||||
Scattered disc: Sedna | |||||||
Jhaarru | Lists of periodic and non-periodic comets Damocloids · Hills baadal · Oort baadal | ||||||
See also the list of solar system objects |
- ↑ "Eris". Lexico UK English Dictionary. Oxford University Press. Archived from the original on July 31, 2020.
- ↑ Noah Webster (1884) A Practical Dictionary of the English Language
- ↑ Ian Douglas (2013) Semper Human
- ↑ "Eris Facts". Space Facts. Archived from the original on May 28, 2023. Retrieved May 26, 2021.
- ↑ Cite error: Invalid
<ref>
tag; no text was provided for refs namedSnodgrass et al. 2010
- ↑ "Dwarf Planets". Canadian Space Agency. March 12, 2020. Archived from the original on November 26, 2020. Retrieved January 1, 2023.