"ടൈറ്റാനിയ" എന്ന താളിന്റെ പതിപ്പുകൾ തമ്മിലുള്ള വ്യത്യാസം

No edit summary
വരി 4:
| alt_names = Uranus III
| adjectives = Titanian
| pronounced = {{IPAc-en|t|ɨ|ˈ|t|ɑː|n|j|ə}} or {{IPAc-en|t|aɪ|ˈ|t|eɪ|n|i|ə}}{{efn | {{respell|ti|TAH|nyə}} or {{respell|ty|TAY|nee-ə}}.<ref name="Webster" /> The former pronunciation is distinct from the adjectival form of Saturn's moon [[Titan (moon)|Titan]].}}
| image = [[File:Titania (moon) color cropped.jpg|260px|alt=A round spherical body is almost fully illuminated. The surface has a mottled appearance with bright patches among relatively dark terrain. The terminator is located near the right edge. A large crater can be seen at the terminator in the upper half of the image. Another bright crater can be seen at the bottom. A large canyon runs from the darkness at the lower-right side to visible center of the body.]]
| caption = ''Voyager 2'' image of Titania's southern hemisphere{{refn | Along the terminator are visible the moon's largest known [[impact crater]], [[Gertrude (crater)|Gertrude]], at upper right and several enormous canyon-like [[graben]]s (the [[Messina Chasma]]ta above, [[Belmont Chasma]] near bottom) at lower right.| group = caption}}
| discovery = yes
| discoverer = [[William Herschel]]
| discovered = January 11, 1787<ref name="Herschel 1787" />
| semimajor = {{val|435910|u=km}}<ref name="orbit" />
| eccentricity = {{val|0.0011}}<ref name="orbit" />
| period = {{val|8.706234|u=d}}<ref name="orbit" />
| avg_speed = 3.64 km/s{{efn|name=calculated|Calculated on the basis of other parameters.}}
| inclination = {{val|0.340|u=°}} (to Uranus's equator)<ref name="orbit" />
| satellite_of = [[Uranus]]
| physical_characteristics = yes
| mean_radius = {{val|788.4|0.6|u=km}} ({{val|0.1235|u=Earths}})<ref name="Widemann Sicardy et al. 2009" />
| surface_area = {{val|7820000|u=km²}}{{efn | Surface area derived from the radius ''r'' : 4π''r''². }}
| volume = {{val|2065000000|u=km³}}{{efn | Volume ''v'' derived from the radius ''r'' : 4π''r''³/3. }}
| mass = {{val|3.527|0.09|e=21|u=kg}} ({{val|5.908|e=-4|u=Earths}})<ref name="Jacobson Campbell et al. 1992" />
| density = {{val|1.711|0.005|u=g/cm³}}<ref name="Widemann Sicardy et al. 2009" />
| surface_grav = {{Gr|3.527|788.4|3}} [[Acceleration|m/s²]]{{efn | Surface gravity derived from the mass ''m'', the [[gravitational constant]] ''G'' and the radius ''r'' : ''Gm/r''². }}
| escape_velocity = {{V2|3.527|788.4}} km/s{{efn | Escape velocity derived from the mass ''m'', the [[gravitational constant]] ''G'' and the radius ''r'' : {{math|{{radical|2Gm/r}}}}. }}
| rotation = presumed [[synchronous rotation|synchronous]]<ref name="Smith Soderblom et al. 1986" />
| albedo =
{{plainlist |
* 0.35 (geometrical)
* 0.17 (Bond)<ref name="Karkoschka, Hubble 2001" />
}}
| magnitude = 13.9<ref name="Newton Teece 1995" />
| temp_name1 = solstice<ref name="Widemann Sicardy et al. 2009" />
| mean_temp_1 = {{nowrap|70 ± 7}}&nbsp;[[Kelvin|K]]
| max_temp_1 = 89&nbsp;K
വരി 65:
==ഇതും കാണൂ==
==അവലംബം==
{{reflist}}
"https://ml.wikipedia.org/wiki/ടൈറ്റാനിയ" എന്ന താളിൽനിന്ന് ശേഖരിച്ചത്