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47:
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1282:) consisting of relatively fresh ice. All large craters on Titania have flat floors and central peaks. The only exception is Ursula, which has a pit in the center. To the west of Gertrude there is an area with irregular topography, the so-called "unnamed basin", which may be another highly degraded impact basin with the diameter of about 330 kilometres (210 mi).
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1008:. This is important, because the trailing hemispheres of satellites orbiting inside a magnetosphere are struck by magnetospheric plasma, which co-rotates with the planet. This bombardment may lead to the darkening of the trailing hemispheres, which is actually observed for all Uranian moons except Oberon (see below).
1317:
relatively low number of impact craters on the moon's present-day surface. Additional episodes of resurfacing may have occurred later and led to the formation of smooth plains. Alternatively smooth plains may be ejecta blankets of the nearby impact craters. The most recent endogenous processes were mainly
2928:
Widemann, T.; Sicardy, B.; Dusser, R.; Martinez, C.; Beisker, W.; Bredner, E.; Dunham, D.; Maley, P.; Lellouch, E.; Arlot, J. -E.; Berthier, J.; Colas, F.; Hubbard, W. B.; Hill, R.; Lecacheux, J.; Lecampion, J. -F.; Pau, S.; Rapaport, M.; Roques, F.; Thuillot, W.; Hills, C. R.; Elliott, A. J.; Miles,
2477:
and
Titania was only 365,200 km (226,900 mi), the best images of this moon have a spatial resolution of about 3.4 km (only Miranda and Ariel were imaged with a better resolution). The images cover about 40% of the surface, but only 24% was photographed with the precision required for
1226:
and along some grabens are somewhat redder. There may be an asymmetry between the leading and trailing hemispheres; the former appears to be redder than the latter by 8%. However, this difference is related to the smooth plains and may be accidental. The reddening of the surfaces probably results
1069:
Titania is the largest and most massive
Uranian moon, the eighth most massive moon in the Solar System, and the 20th largest object in the Solar System. Its density of 1.68 g/cm, which is much higher than the typical density of Saturn's satellites, indicates that it consists of roughly equal
1316:
formation and endogenic resurfacing. The former acted over the moon's entire history and influenced all surfaces. The latter processes were also global in nature, but active mainly for a period following the moon's formation. They obliterated the original heavily cratered terrain, explaining the
2422:
Titania's accretion probably lasted for several thousand years. The impacts that accompanied accretion caused heating of the moon's outer layer. The maximum temperature of around 250 K (−23 °C) was reached at a depth of about 60 kilometres (37 mi). After the end of formation, the
1133:
radiation or energetic charged particles coming from the magnetosphere of Uranus. The latter process would explain the asymmetry in its distribution, because the trailing hemisphere is subject to a more intense magnetospheric influence than the leading hemisphere. Another possible source is the
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of this mixture is 176 K (−97 °C). If the temperature dropped below this value, the ocean would have subsequently frozen. The freezing of the water would have caused the interior to expand, which may have been responsible for the formation of the majority of the canyons. However, the
2366:
is a steep function of temperature, this may lead to the accumulation of carbon dioxide in the low-latitude regions of
Titania, where it can stably exist on high albedo patches and shaded regions of the surface in the form of ice. During the summer, when the polar temperatures reach as high as
1097:
are slightly stronger on
Titania's leading hemisphere than on the trailing hemisphere. This is the opposite of what is observed on Oberon, where the trailing hemisphere exhibits stronger water ice signatures. The cause of this asymmetry is not known, but it may be related to the bombardment by
1297:, which runs for about 1,500 kilometres (930 mi) from the equator almost to the south pole. The grabens on Titania are 20–50 kilometres (12–31 mi) wide and have a relief of about 2–5 km. The scarps that are not related to canyons are called rupes, such as
1161:. If this is the case, the radius of the core 520 kilometres (320 mi) is about 66% of the radius of the moon, and its mass is around 58% of the moon's mass—the proportions are dictated by moon's composition. The pressure in the center of Titania is about 0.58
796:. He later reported the discoveries of four more satellites, although they were subsequently revealed as spurious. For nearly the next 50 years, Titania and Oberon would not be observed by any instrument other than William Herschel's, although the moon can be seen from
1185:
of 176 K). However the present internal structure of
Titania depends heavily on its thermal history, which is poorly known. Recent studies suggest, contrary to earlier theories, that Uranus largest moons like Titania in fact could have active subsurface oceans.
1305:'s image resolution. These smooth plains were probably resurfaced later in Titania's geological history, after the majority of craters formed. The resurfacing may have been either endogenic in nature, involving the eruption of fluid material from the interior (
2453:
present knowledge of
Titania's geological evolution is quite limited. Whereas more up to date analysis suggest that larger moons of Uranus are not only capable of having active subsurface oceans; but in fact; presumed to have subterranean oceans beneath them.
2375:. The accumulated carbon dioxide ice can be removed from cold traps by magnetospheric particles, which sputter it from the surface. Titania is thought to have lost a significant amount of carbon dioxide since its formation 4.6 billion years ago.
2447:
was present. Further melting may have led to the separation of ice from rocks and formation of a rocky core surrounded by an icy mantle. A layer of liquid water (ocean) rich in dissolved ammonia may have formed at the core–mantle boundary. The
2518:. The science questions motivating this prioritization include questions about the Uranian satellites' bulk properties, internal structure, and geologic history. A Uranus orbiter was listed as the third priority for a NASA
1266:). The surface of Titania is less heavily cratered than the surfaces of either Oberon or Umbriel, which means that the surface is much younger. The crater diameters reach 326 kilometers for the largest known crater,
2431:
in the moon's crust leading to cracking. Some of the present-day canyons may be a result of this. The process lasted for about 200 million years, implying that any endogenous activity ceased billions of years ago.
2355:. This upper limit is still several times higher than the maximum possible surface pressure of the carbon dioxide, meaning that the measurements place essentially no constraints on parameters of the atmosphere.
3254:"On the Discovery of Four Additional Satellites of the Georgium Sidus. The Retrograde Motion of Its Old Satellites Announced; And the Cause of Their Disappearance at Certain Distances from the Planet Explained"
1309:), or, alternatively it may be due to blanking by the impact ejecta from nearby large craters. The grabens are probably the youngest geological features on Titania—they cut all craters and even smooth plains.
866:, although he sometimes used William Herschel's numbering (where Titania and Oberon are II and IV). In 1851 Lassell eventually numbered all four known satellites in order of their distance from the planet by
744:, outermost of the five large moons of Uranus. It may have undergone an early endogenic resurfacing event which obliterated its older, heavily cratered surface. Its surface is cut by a system of enormous
4498:
Committee on the
Planetary Science and Astrobiology Decadal Survey; Space Studies Board; Division on Engineering and Physical Sciences; National Academies of Sciences, Engineering, and Medicine (2022).
1011:
Because Uranus orbits the Sun almost on its side, and its moons orbit in the planet's equatorial plane, they (including
Titania) are subject to an extreme seasonal cycle. Both northern and southern
6119:
973:
Titania orbits Uranus at the distance of about 436,000 kilometres (271,000 mi), being the second farthest from the planet among its five major moons after Oberon. Titania's orbit has a small
3906:
Jacobson, R. A.; Campbell, J. K.; Taylor, A. H.; Synnott, S. P. (June 1992). "The masses of Uranus and its major satellites from
Voyager tracking data and earth-based Uranian satellite data".
1321:
in nature and caused the formation of the canyons, which are actually giant cracks in the ice crust. The cracking of the crust was caused by the global expansion of
Titania by about 0.7%.
2347:, and to detect any extant atmosphere. The data revealed no atmosphere to a surface pressure of 1–2 mPa (10–20 nbar); if it exists, it would have to be far thinner than that of
183:
5444:
3758:
Ness, Norman F.; Acuña, Mario H.; Behannon, Kenneth W.; Burlaga, Leonard F.; Connerney, John E. P.; Lepping, Ronald P.; Neubauer, Fritz M. (July 1986). "Magnetic Fields at Uranus".
2387:
or subnebula; a disc of gas and dust that either existed around Uranus for some time after its formation or was created by the giant impact that most likely gave Uranus its large
778:
put an upper limit on the surface pressure of any possible atmosphere at 1–2 mPa (10–20 nbar). The Uranian system has been studied up close only once, by the spacecraft
1035:
of Uranus's moons become possible. In 2007–2008 a number of such events were observed including two occultations of Titania by Umbriel on August 15 and December 8, 2007.
3351:
1027:
flyby coincided with the southern hemisphere's 1986 summer solstice, when nearly the entire southern hemisphere was illuminated. Once every 42 years, when Uranus has an
6255:
4542:
2320:, are unlikely to be present, because Titania's weak gravity could not prevent them from escaping into space. At the maximum temperature attainable during Titania's
1660:
1239:. However, the color asymmetry of Titania is more likely related to accretion of a reddish material coming from outer parts of the Uranian system, possibly, from
2930:
5437:
4020:. Lunar and Planetary Science Conference, 21st, March 12–16, 1990. Houston, TX, United States: Lunar and Planetary Sciences Institute. pp. 473–489.
752:, the result of the expansion of its interior during the later stages of its evolution. Like all major moons of Uranus, Titania probably formed from an
1125:, which is concentrated mainly on the trailing hemisphere. The origin of the carbon dioxide is not completely clear. It might be produced locally from
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5069:
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1177:
at the core–mantle boundary. The thickness of this ocean, if it exists, is up to 50 kilometres (31 mi) and its temperature is around 190
2988:"The Uranus system from occultation observations (1977–2006): Rings, pole direction, gravity field, and masses of Cressida, Cordelia, and Ophelia"
2439:
together with continued decay of radioactive elements were probably strong enough to melt the ice if some antifreeze like ammonia (in the form of
4434:
2391:. The precise composition of the subnebula is not known; however, the relatively high density of Titania and other Uranian moons compared to the
1198:
Titania with some surface features labeled. The south pole is situated close to the unlabeled bright crater below and left of the crater Jessica.
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The color is determined by the ratio of albedos viewed through the green (0.52–0.59 μm) and violet (0.38–0.45 μm) Voyager filters.
6265:
5316:
3077:
Smith, B. A.; Soderblom, L. A.; Beebe, A.; Bliss, D.; Boyce, J. M.; Brahic, A.; Briggs, G. A.; Brown, R. H.; Collins, S. A. (4 July 1986).
4645:"From Titania to large trans-Neptunian objects: ground-based stellar occultations in the quest for the billionth of atmospheric pressure"
4340:
Squyres, S. W.; Reynolds, Ray T.; Summers, Audrey L.; Shung, Felix (1988). "Accretional Heating of the Satellites of Saturn and Uranus".
5362:
4644:
4619:
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Miller, C.; Chanover, N. J. (March 2009). "Resolving dynamic parameters of the August 2007 Titania and Ariel occultations by Umbriel".
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2016:
1967:
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French, Richard G.; Hedman, Matthew M.; Nicholson, Philip D.; Longaretti, Pierre-Yves; McGhee-French, Colleen A. (2024-03-15).
2503:
concept, evaluated around 2010. Uranus was also examined as part of one trajectory for a precursor interstellar probe concept,
1709:
853:, the year before. It is uncertain if Herschel devised the names, or if Lassell did so and then sought Herschel's permission.
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238:
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3697:
Grundy, W. M.; Young, L. A.; Spencer, J. R.; Johnson, R. E.; Young, E. F.; Buie, M. W. (October 2006). "Distributions of H
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1202:
Among Uranus's moons, Titania is intermediate in brightness between the dark Oberon and Umbriel and the bright Ariel and
792:
Titania was discovered by William Herschel on January 11, 1787, the same day he discovered Uranus's second largest moon,
5517:
4420:
4104:
Buratti, Bonnie J.; Mosher, Joel A. (March 1991). "Comparative global albedo and color maps of the Uranian satellites".
2857:(audio CD). The second is used by interviewees in a podcast by the Folger Shakespeare Library, but not by the narrator:
1488:
1012:
833:
701:
2929:
R.; Platt, T.; Cremaschini, C.; Dubreuil, P.; Cavadore, C.; Demeautis, C.; Henriquet, P.; et al. (February 2009).
2829:
2482:. At the time of the flyby, the southern hemisphere of Titania (like those of the other moons) was pointed towards the
2004:
1015:
spend 42 years in a complete darkness, and another 42 years in continuous sunlight, with the sun rising close to the
5927:
4385:
Hillier, John; Squyres, Steven W. (August 1991). "Thermal stress tectonics on the satellites of Saturn and Uranus".
3505:
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4296:"Modeling the thermodynamical conditions in the Uranian subnebula – Implications for regular satellite composition"
2540:
1643:
732:. Its surface, which is relatively dark and slightly red in color, appears to have been shaped by both impacts and
2473:
probe, which photographed the moon during its flyby of Uranus in January 1986. Since the closest distance between
1102:, which is stronger on the trailing hemisphere (due to the plasma's co-rotation). The energetic particles tend to
2427:
present in its rocks. The cooling near-surface layer contracted, while the interior expanded. This caused strong
4056:
Plescia, J. B. (December 30, 1987). "Cratering history of the Uranian satellites: Umbriel, Titania and Oberon".
3954:"Subsurface oceans and deep interiors of medium-sized outer planet satellites and large trans-neptunian objects"
2304:
The presence of carbon dioxide on the surface suggests that Titania may have a tenuous seasonal atmosphere of CO
729:
6159:
5055:
4993:
4867:
2961:
2500:
2436:
2053:
774:
with a surface pressure of about 10 nanopascals (10 bar). Measurements during Titania's occultation of a
3140:(2001). "Comprehensive Photometry of the Rings and 16 Satellites of Uranus with the Hubble Space Telescope".
6250:
2840:
1222:. However, fresh impact deposits are bluer, while the smooth plains situated on the leading hemisphere near
1099:
856:
Titania was initially referred to as "the first satellite of Uranus", and in 1848 was given the designation
458:
329:
1121:
Except for water, the only other compound identified on the surface of Titania by infrared spectroscopy is
2858:
2651:
2623:
2309:
1430:
1367:
2763:, a Saturnian moon, has the density of 0.97 g/cm, which implies it contains more than 90% of water.
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2462:
828:
574:
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in January 1986. It took several images of Titania, which allowed mapping of about 40% of its surface.
2987:
2931:"Titania's radius and an upper limit on its atmosphere from the September 8, 2001 stellar occultation"
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3401:
3360:
3314:
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3149:
3090:
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2102:
1859:
1704:
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1289:, or scarps. In some places, two parallel scarps mark depressions in the satellite's crust, forming
6234:
6139:
5688:
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4907:
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Surface features on Titania are named for female characters or locations from Shakespeare's works.
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1139:
1115:
978:
820:
298:
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A Uranus orbiter and probe mission architecture was identified as the highest priority for a NASA
2415:
and methane. The moons that formed in such a subnebula would contain less water ice (with CO and N
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4890:
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1270:(there can be also a degraded basin of approximately the same size). Some craters (for instance,
537:
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803:
46:
1169:). The current state of the icy mantle is unclear. If the ice contains enough ammonia or other
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Origins, Worlds, and Life: A Decadal Strategy for Planetary Science and Astrobiology 2023-2032
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Strobell, M.E.; Masursky, H. (1987). "New Features Named on the Moon and Uranian Satellites".
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reaching up to 326 kilometres (203 mi) in diameter, but is less heavily cratered than
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3846:"Observation of an eclipse of U-3 Titania by U-2 Umbriel on December 8, 2007 with ESO-VLT"
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on from Saturn to Uranus in an extended mission. Another mission concept proposed was the
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and migrates to the opposite pole and to the equatorial regions, giving rise to a type of
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837:. The names of all four satellites of Uranus then known were suggested by Herschel's son
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of about 17%. Its surface is generally slightly red in color, but less red than that of
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The peculiar geometry of the Uranian system causes the moons' poles to receive more
1293:, which are sometimes called canyons. The most prominent among Titania's canyons is
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3118:
2790:"An Account of the Discovery of Two Satellites Revolving Round the Georgian Planet"
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near Ursula crater. The regions along some scarps and near Ursula appear smooth at
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proportions of water ice and dense non-ice components; the latter could be made of
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s highest-resolution image of Titania shows moderately cratered plains, enormous
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4243:. Vol. 20. Lunar and Planetary Sciences Institute, Houston. p. 205C.
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from the interior may be related to the past geological activity on this moon.
1043:
6124:
5824:
5794:
5775:
5717:
5682:
5271:
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4237:
New geological maps of Uranian satellites Titania, Oberon, Umbriel and Miranda
4018:
A search for spectral units on the Uranian satellites using color ratio images
2423:
subsurface layer cooled, while the interior of Titania heated due to decay of
2395:
indicates that it may have been relatively water-poor. Significant amounts of
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1170:
1135:
1103:
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771:
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2165:
2129:
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2080:
2067:
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2018:
1982:
1969:
1933:
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2526:, and conceptual designs for such a mission are currently being analyzed.
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Scientists have recognized three classes of geological feature on Titania:
5523:
3705:
ices on Ariel, Umbriel, Titania, and Oberon from IRTF/SpeX observations".
57:, January 1986. Along the terminator are visible the moon's largest known
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1020:
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trapped as a clathrate) and more rock, explaining their higher density.
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spectroscopy conducted from 2001 to 2005 revealed the presence of water
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of 7.2; this was an opportunity to both refine Titania's diameter and
770:
on Titania's surface, suggesting it may have a tenuous carbon dioxide
5558:
5090:
4987:
4723:
3616:(December 1851). "Letter from William Lassell, Esq., to the Editor".
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1178:
1075:
1016:
745:
706:
522:
472:
372:
316:
66:
4500:
3253:
3078:
2892:
2489:
No other spacecraft has ever visited the Uranian system or Titania.
1243:, which would be deposited predominately on the leading hemisphere.
1061:. Near the bottom, a region of smoother plains including the crater
6193:
4510:
3927:
3637:
3414:
3389:
3004:
6073:
5047:
3719:
2352:
1495:
1425:
1362:
1323:
1259:
1251:
1193:
1042:
808:
802:
797:
5988:
5476:
4559:, Jet Propulsion Laboratory/California Institute of Technology,
4187:
4154:
2750:
on the surface of Callisto is about 10 nPa (10 pbar).
2717:
2444:
1166:
1054:
812:
775:
394:
5426:
5051:
4696:
4335:
4333:
4331:
3072:
3070:
3068:
2895:. Jet Propulsion Laboratory, California Institute of Technology
2362:
than their equatorial regions. Because the vapor pressure of CO
1312:
The geology of Titania was influenced by two competing forces:
1214:) to 25% at an angle of about 1°. Titania has a relatively low
4191:
4158:
3066:
3064:
3062:
3060:
3058:
3056:
3054:
3052:
3050:
3048:
2923:
2921:
2919:
2917:
2915:
2913:
2911:
2909:
2483:
2467:
So far the only close-up images of Titania have been from the
1210:: its reflectivity decreases from 35% at a phase angle of 0° (
1162:
763:
4620:"Is there an atmosphere around Titania, satellite of Uranus?"
4149:
4147:
4145:
4143:
3952:
Hussmann, Hauke; Sohl, Frank; Spohn, Tilman (November 2006).
627:
206:
135:
3947:
3945:
3943:
3941:
3939:
3937:
3692:
3690:
3688:
1146:
trapped by water ice in Titania's interior. The escape of CO
1001:
satellite, with one face always pointing toward the planet.
819:
All of Uranus's moons are named after characters created by
679:. At a diameter of 1,578 kilometres (981 mi) it is the
3686:
3684:
3682:
3680:
3678:
3676:
3674:
3672:
3670:
3668:
3437:
Lassell, W. (1852). "Beobachtungen der Uranus-Satelliten".
941:
938:
932:
923:
906:
897:
716:
Titania consists of approximately equal amounts of ice and
663:
660:
654:
645:
636:
633:
618:
215:
212:
197:
171:
168:
162:
153:
144:
141:
126:
4574:"Uranus, Neptune in NASA’s sights for new robotic mission"
3132:
3130:
3128:
3079:"Voyager 2 in the Uranian System: Imaging Science Results"
2486:, so the northern (dark) hemisphere could not be studied.
4692:
3994:"New Study of Uranus' Large Moons Shows 4 May Hold Water"
3258:
Philosophical Transactions of the Royal Society of London
3214:
Philosophical Transactions of the Royal Society of London
2794:
Philosophical Transactions of the Royal Society of London
2558:
Spelled the same as the adjectival form of Saturn's moon
1285:
Titania's surface is intersected by a system of enormous
903:
888:
4264:
Abstracts of the Lunar and Planetary Science Conference
3844:
Arlot, J. -E.; Dumas, C.; Sicardy, B. (December 2008).
3394:
Publications of the Astronomical Society of the Pacific
2328:
of carbon dioxide is about 300 μPa (3 nbar).
1114:
and darken other organics, leaving a dark, carbon-rich
1129:
or organic materials under the influence of the solar
1031:
and its equatorial plane intersects the Earth, mutual
756:
which surrounded the planet just after its formation.
6170:
935:
900:
657:
630:
218:
209:
165:
138:
4435:"Uranus' large moons may hold water, new study find"
3173:
3171:
2849:
Lexico/OED. Only the first pronunciation is used in
1089:
observations made in 2001–2005, which have revealed
929:
920:
894:
885:
651:
642:
624:
615:
203:
194:
159:
150:
132:
123:
5949:
5582:
5531:
5464:
5309:
5249:
5233:
5226:
5180:
5099:
5011:
4967:
4948:
4929:
4920:
4866:
4850:
4819:
4812:
4774:
4743:
4421:"NASA Says 4 of Uranus' Large Moons May Hold Water"
3888:. Jet Propulsion Laboratory (Solar System Dynamics)
2859:
Brave New Worlds: The Shakespearean Moons of Uranus
1004:Titania's orbit lies completely inside the Uranian
926:
891:
648:
621:
573:
552:
547:
535:
471:
456:
444:
429:
413:
393:
371:
350:
327:
322:
310:
297:
284:
266:
254:
236:
229:
200:
182:
156:
129:
114:
104:
99:
91:
79:
74:
4557:"Ice Giant Science: The Case for a Uranus Orbiter"
65:, at upper right and several enormous canyon-like
5089:Listed in approximately increasing distance from
4561:Report to the Decadal Survey Giant Planets Panel,
3578:Monthly Notices of the Royal Astronomical Society
3537:Monthly Notices of the Royal Astronomical Society
3469:Monthly Notices of the Royal Astronomical Society
3352:Monthly Notices of the Royal Astronomical Society
3307:Monthly Notices of the Royal Astronomical Society
3042:Jacobson (2023), as cited in French et al. (2024)
4613:NASA archive of publicly released Titania images
1093:water ice on the surface of the moon. Water ice
949:, by analogy with the familiar chemical element
728:. A layer of liquid water may be present at the
4051:
4049:
4047:
4045:
4043:
4041:
4039:
4037:
4035:
2780:
2778:
1231:caused by bombardment by charged particles and
965:is ancient Greek for "Daughter of the Titans".
800:with a present-day high-end amateur telescope.
4505:. Washington, D.C.: National Academies Press.
4289:
4287:
4285:
4099:
4097:
4095:
2700:The seven moons more massive than Titania are
720:, and is probably differentiated into a rocky
5438:
5063:
4708:
4230:
4228:
4226:
4224:
4222:
4220:
2893:"Planetary Satellite Mean Orbital Parameters"
989:is around 8.7 days, coincident with its
879:Shakespeare's character's name is pronounced
870:, and since then Titania has been designated
8:
4541:: CS1 maint: multiple names: authors list (
3652:"Merriam-Webster online dictionary: titania"
2853:, e.g. Shakespeare Recording Society (1995)
2571:Calculated on the basis of other parameters.
1082:. The presence of water ice is supported by
687:, with a surface area comparable to that of
39:
4011:
4009:
4007:
4005:
4003:
3210:"On the Georgian Planet and Its Satellites"
3184:. Cambridge University Press. p. 109.
1153:Titania may be differentiated into a rocky
957:, is homonymous with that of Saturn's moon
5445:
5431:
5423:
5230:
5070:
5056:
5048:
4926:
4816:
4715:
4701:
4693:
4241:Proceeding of Lunar and Planetary Sciences
2383:Titania is thought to have formed from an
1331:
1278:) are surrounded by bright impact ejecta (
845:, who had discovered the other two moons,
45:
4618:Sicardy, Bruno; Widemann, Thomas (2001).
4369:
4319:
3886:"Planetary Satellite Physical Parameters"
3869:
3718:
3597:
3556:
3488:
3413:
3372:
3326:
3277:
3233:
3003:
2805:
4163:"Titania Nomenclature Table of Contents"
1328:Messina Chasma—a large canyon on Titania
6256:Astronomical objects discovered in 1787
6177:
2887:
2885:
2883:
2881:
2879:
2774:
2551:
736:processes. It is covered with numerous
4534:
4016:Bell III, J.F.; McCord, T. B. (1991).
3533:"Observations of Satellites of Uranus"
3465:"On the interior satellites of Uranus"
2646:Escape velocity derived from the mass
2618:Surface gravity derived from the mass
1065:is split by the graben Belmont Chasma.
38:
4450:"The Voyager 2 Encounter with Uranus"
2580:Surface area derived from the radius
2403:may have been present in the form of
2292:
7:
4688:USGS Planetary Nomenclature web site
3178:Newton, Bill; Teece, Philip (1995).
2562:, but may be pronounced differently.
2308:, much like that of the Jovian moon
4202:. USGS Astrogeology. Archived from
4200:Gazetteer of Planetary Nomenclature
4167:Gazetteer of Planetary Nomenclature
3506:"The Shakespearean Moons of Uranus"
914:, but the moon is often pronounced
4448:Stone, E. C. (December 30, 1987).
3303:"Note on the Satellites of Uranus"
1333:Named surface features on Titania
1039:Composition and internal structure
827:. The name Titania was taken from
25:
6228:
6216:
6204:
6192:
6180:
5522:
5516:
5510:
5032:
5031:
2524:Planetary Science Decadal Survey
2516:Planetary Science Decadal Survey
2505:Innovative Interstellar Explorer
916:
881:
611:
190:
119:
6261:Discoveries by William Herschel
4457:Journal of Geophysical Research
4387:Journal of Geophysical Research
4342:Journal of Geophysical Research
4058:Journal of Geophysical Research
3390:"The Fifth Satellite of Uranus"
1710:The Life and Death of King John
993:. In other words, Titania is a
695:in 1787, it is named after the
3181:The guide to amateur astronomy
2331:On September 8, 2001, Titania
1019:over one of the poles at each
1:
4858:Uranus-crossing minor planets
3574:"Bright Satellites of Uranus"
3347:"On the Satellites of Uranus"
2493:, now discarded, was to send
2367:85–90 K, carbon dioxide
1206:. Its surface shows a strong
4596:. NASA. 1999. Archived from
4300:Astronomy & Astrophysics
4126:10.1016/0019-1035(91)90064-Z
3980:10.1016/j.icarus.2006.06.005
3831:10.1016/j.icarus.2008.12.010
3737:10.1016/j.icarus.2006.04.016
3512:. Folger Shakespeare Library
3022:10.1016/j.icarus.2024.115957
2958:10.1016/j.icarus.2008.09.011
2871:Anthony Burgess: A Biography
1181:(close to the water–ammonia
981:very little relative to the
6266:Moons with a prograde orbit
3871:10.1051/0004-6361:200810134
3780:10.1126/science.233.4759.85
3103:10.1126/science.233.4759.43
2005:The Two Gentlemen of Verona
1098:charged particles from the
841:in 1852, at the request of
6282:
4321:10.1051/0004-6361:20031515
3850:Astronomy and Astrophysics
2746:The partial pressure of CO
2541:List of natural satellites
2460:
1548:
29:
6115:
5508:
5085:
5027:
4730:
4679:Views of the Solar System
4643:Widemann, Thomas (2009).
3439:Astronomische Nachrichten
2851:A Midsummer Night's Dream
2679:The five major moons are
2243:
2194:
2145:
2096:
2047:
1998:
1949:
1902:
1853:
1806:
1752:
1700:
1639:
1590:
1536:
1489:All's Well That Ends Well
1473:
1415:
1373:
1354:
1349:
1346:
1343:
1340:
1337:
1078:material including heavy
834:A Midsummer Night's Dream
702:A Midsummer Night's Dream
490:
269:Orbital period (sidereal)
44:
5967:: 5268 km / 0.413 Earths
4994:Uranus Orbiter and Probe
4463:(A13): 14, 873–14, 876.
4064:(A13): 14, 918–14, 932.
3908:The Astronomical Journal
2601:derived from the radius
2501:Uranus orbiter and probe
2054:Pericles, Prince of Tyre
829:the Queen of the Fairies
705:. Its orbit lies inside
323:Physical characteristics
30:Not to be confused with
4477:10.1029/JA092iA13p14873
4393:(E1): 15, 665–15, 674.
4362:10.1029/JB093iB08p08779
4312:2004A&A...413..373M
4078:10.1029/JA092iA13p14918
3862:2008A&A...492..599A
3654:. Merriam-Webster. 2009
2841:Oxford University Press
1100:magnetosphere of Uranus
953:. The adjectival form,
459:Synodic rotation period
231:Orbital characteristics
3599:10.1093/mnras/10.6.135
3504:Paul, Richard (2014).
3388:Kuiper, G. P. (1949).
3279:10.1098/rstl.1798.0005
3235:10.1098/rstl.1788.0024
3162:10.1006/icar.2001.6596
2807:10.1098/rstl.1787.0016
2691:, Titania and Oberon.
2652:gravitational constant
2624:gravitational constant
2202:Much Ado About Nothing
1908:The Merchant of Venice
1431:Much Ado About Nothing
1368:The Merchant of Venice
1347:Length (diameter), km
1329:
1199:
1066:
816:
51:Titania, as imaged by
27:Largest moon of Uranus
4235:Croft, S. K. (1989).
4196:"Gertrude on Titania"
3490:10.1093/mnras/12.1.15
3250:Herschel, William Sr.
2837:UK English Dictionary
2463:Exploration of Uranus
1327:
1197:
1173:, Titania may have a
1157:surrounded by an icy
1106:water ice, decompose
1046:
806:
575:Composition by volume
306:(to Uranus's equator)
18:Atmosphere of Titania
6140:Planetary-mass moons
4684:Titania nomenclature
3618:Astronomical Journal
3572:Lassell, W. (1850).
3558:10.1093/mnras/8.3.43
3531:Lassell, W. (1848).
3463:Lassell, W. (1851).
3374:10.1093/mnras/3.5.35
3328:10.1093/mnras/8.3.43
2450:eutectic temperature
2429:extensional stresses
2425:radioactive elements
2379:Origin and evolution
2312:. Other gases, like
1860:Antony and Cleopatra
1705:Eleanor of Aquitaine
1543:The Comedy of Errors
1241:irregular satellites
1235:over the age of the
1183:eutectic temperature
788:Discovery and naming
730:core–mantle boundary
697:queen of the fairies
5310:Geological features
4908:(472651) 2015 DB216
4469:1987JGR....9214873S
4399:1991JGR....9615665H
4354:1988JGR....93.8779S
4294:Mousis, O. (2004).
4276:1987LPI....18..964S
4249:1989LPI....20..205C
4194:(October 1, 2006).
4169:. USGS Astrogeology
4118:1991Icar...90....1B
4070:1987JGR....9214918P
4026:1991LPSC...21..473B
3972:2006Icar..185..258H
3920:1992AJ....103.2068J
3823:2009Icar..200..343M
3772:1986Sci...233...85N
3729:2006Icar..184..543G
3630:1851AJ......2...70L
3590:1850MNRAS..10..135L
3549:1848MNRAS...8...43L
3481:1851MNRAS..12...15L
3451:1852AN.....34..325.
3406:1949PASP...61..129K
3365:1834MNRAS...3...35H
3319:1848MNRAS...8...43L
3301:Struve, O. (1848).
3270:1798RSPT...88...47H
3226:1788RSPT...78..364H
3154:2001Icar..151...51K
3095:1986Sci...233...43S
3014:2024Icar..41115957F
2950:2009Icar..199..458W
2437:accretional heating
2273: /
2224: /
2175: /
2126: /
2077: /
2028: /
1979: /
1930: /
1883: /
1834: /
1787: /
1733: /
1672: /
1620: /
1571: /
1517: /
1454: /
1396: /
1334:
821:William Shakespeare
807:Size comparison of
681:eighth largest moon
671:), also designated
92:Discovery date
41:
6120:Discovery timeline
5454:Natural satellites
3252:(1 January 1798).
3208:(1 January 1788).
2536:Titania in fiction
2480:geological mapping
1332:
1330:
1212:geometrical albedo
1200:
1110:trapped in ice as
1067:
817:
766:as well as frozen
538:Apparent magnitude
480:0.35 (geometrical)
344:0.1235 Earths
81:Discovered by
6168:
6167:
5968:
5420:
5419:
5305:
5304:
5227:Outer (irregular)
5045:
5044:
5007:
5006:
4999:Uranus Pathfinder
4916:
4915:
4649:Paris Observatory
4624:Paris Observatory
4594:"Titania profile"
4555:Mark Hofstadter,
4520:978-0-309-47578-5
4407:10.1029/91JE01401
4348:(B8): 8779–8794.
3191:978-0-521-44492-7
3138:Karkoschka, Erich
2847:on March 2, 2020.
2522:by the 2013-2022
2514:by the 2023–2032
2341:visible magnitude
2324:(89 K), the
2297:
2296:
2103:The Winter's Tale
1688:Calphurnia crater
1644:Calpurnia Pisonis
1112:clathrate hydrate
1080:organic compounds
991:rotational period
699:in Shakespeare's
675:, is the largest
604:
603:
531:
530:
312:Satellite of
16:(Redirected from
6273:
6233:
6232:
6231:
6221:
6220:
6219:
6209:
6208:
6207:
6197:
6196:
6185:
6184:
6183:
6176:
5963:
5942:
5930:
5916:
5902:
5885:
5873:
5866:
5847:
5833:
5819:
5784:
5770:
5756:
5751:
5729:
5724:
5712:
5705:
5691:
5677:
5660:
5643:
5633:
5624:
5610:
5526:
5520:
5514:
5447:
5440:
5433:
5424:
5378:Messina Chasmata
5322:Kachina Chasmata
5231:
5181:Major (spheroid)
5072:
5065:
5058:
5049:
5035:
5034:
4927:
4896:
4886:
4827:William Herschel
4817:
4717:
4710:
4703:
4694:
4664:
4662:
4660:
4651:. Archived from
4639:
4637:
4635:
4630:on March 7, 2013
4626:. Archived from
4609:
4607:
4605:
4600:on June 13, 2009
4581:
4578:Spaceflight Now,
4570:
4564:
4553:
4547:
4546:
4540:
4532:
4495:
4489:
4488:
4454:
4445:
4439:
4438:
4431:
4425:
4424:
4417:
4411:
4410:
4382:
4376:
4375:
4373:
4371:2060/19870013922
4337:
4326:
4325:
4323:
4291:
4280:
4279:
4259:
4253:
4252:
4232:
4215:
4214:
4212:
4211:
4184:
4178:
4177:
4175:
4174:
4151:
4138:
4137:
4101:
4090:
4089:
4053:
4030:
4029:
4013:
3998:
3997:
3990:
3984:
3983:
3949:
3932:
3931:
3914:(6): 2068–2078.
3903:
3897:
3896:
3894:
3893:
3882:
3876:
3875:
3873:
3841:
3835:
3834:
3806:
3800:
3799:
3755:
3749:
3748:
3722:
3694:
3663:
3662:
3660:
3659:
3648:
3642:
3641:
3614:Lassell, William
3610:
3604:
3603:
3601:
3569:
3563:
3562:
3560:
3528:
3522:
3521:
3519:
3517:
3501:
3495:
3494:
3492:
3460:
3454:
3453:
3434:
3428:
3427:
3417:
3385:
3379:
3378:
3376:
3339:
3333:
3332:
3330:
3298:
3292:
3291:
3281:
3246:
3240:
3239:
3237:
3202:
3196:
3195:
3175:
3166:
3165:
3134:
3123:
3122:
3074:
3043:
3040:
3034:
3033:
3007:
2983:
2977:
2976:
2974:
2972:
2967:on July 25, 2014
2966:
2960:. Archived from
2935:
2925:
2904:
2903:
2901:
2900:
2889:
2874:
2867:
2861:
2848:
2843:. Archived from
2826:
2820:
2819:
2809:
2782:
2764:
2757:
2751:
2744:
2738:
2735:
2729:
2698:
2692:
2677:
2671:
2669:
2668:
2667:
2644:
2638:
2616:
2610:
2595:
2589:
2578:
2572:
2569:
2563:
2556:
2520:Flagship mission
2512:Flagship mission
2288:
2287:
2285:
2284:
2283:
2278:
2274:
2271:
2270:
2269:
2266:
2239:
2238:
2236:
2235:
2234:
2229:
2225:
2222:
2221:
2220:
2217:
2190:
2189:
2187:
2186:
2185:
2180:
2176:
2173:
2172:
2171:
2168:
2141:
2140:
2138:
2137:
2136:
2131:
2127:
2124:
2123:
2122:
2119:
2092:
2091:
2089:
2088:
2087:
2082:
2078:
2075:
2074:
2073:
2070:
2043:
2042:
2040:
2039:
2038:
2033:
2029:
2026:
2025:
2024:
2021:
1994:
1993:
1991:
1990:
1989:
1984:
1980:
1977:
1976:
1975:
1972:
1945:
1944:
1942:
1941:
1940:
1935:
1931:
1928:
1927:
1926:
1923:
1898:
1897:
1895:
1894:
1893:
1888:
1884:
1881:
1880:
1879:
1876:
1849:
1848:
1846:
1845:
1844:
1839:
1835:
1832:
1831:
1830:
1827:
1802:
1801:
1799:
1798:
1797:
1792:
1788:
1785:
1784:
1783:
1780:
1748:
1747:
1745:
1744:
1743:
1738:
1734:
1731:
1730:
1729:
1726:
1696:
1695:
1693:
1692:
1691:
1689:
1684:
1683:
1678:
1673:
1670:
1669:
1668:
1665:
1635:
1634:
1632:
1631:
1630:
1625:
1621:
1618:
1617:
1616:
1613:
1597:Henry VI, Part 3
1586:
1585:
1583:
1582:
1581:
1576:
1572:
1569:
1568:
1567:
1564:
1532:
1531:
1529:
1528:
1527:
1522:
1518:
1515:
1514:
1513:
1510:
1469:
1468:
1466:
1465:
1464:
1459:
1455:
1452:
1451:
1450:
1447:
1417:Messina Chasmata
1411:
1410:
1408:
1407:
1406:
1401:
1397:
1394:
1393:
1392:
1389:
1335:
1229:space weathering
1208:opposition surge
1190:Surface features
1175:subsurface ocean
1095:absorption bands
948:
947:
944:
943:
940:
937:
934:
931:
928:
925:
922:
913:
912:
909:
908:
905:
902:
899:
896:
893:
890:
887:
874:
860:
693:William Herschel
691:. Discovered by
670:
669:
666:
665:
662:
659:
656:
653:
650:
647:
644:
639:
638:
635:
632:
629:
626:
623:
620:
617:
520:
492:
491:
424:
409:
407:
403:
389:
387:
384:
381:
367:
365:
362:
345:
341:
339:
305:
280:
278:
262:
250:
248:
225:
224:
221:
220:
217:
214:
211:
208:
205:
202:
199:
196:
178:
177:
174:
173:
170:
167:
164:
161:
158:
155:
152:
147:
146:
143:
140:
137:
134:
131:
128:
125:
95:January 11, 1787
86:William Herschel
49:
42:
21:
6281:
6280:
6276:
6275:
6274:
6272:
6271:
6270:
6241:
6240:
6239:
6229:
6227:
6217:
6215:
6205:
6203:
6191:
6181:
6179:
6171:
6169:
6164:
6130:Irregular moons
6111:
5951:
5945:
5940:
5935:
5926:
5912:
5898:
5883:
5878:
5869:
5862:
5843:
5829:
5815:
5807:Jupiter trojans
5780:
5766:
5754:
5749:
5727:
5722:
5708:
5701:
5687:
5675:
5656:
5641:
5636:
5629:
5620:
5606:
5585:
5578:
5534:
5527:
5521:
5515:
5506:
5467:
5460:
5451:
5421:
5416:
5388:Rousillon Rupes
5301:
5245:
5222:
5176:
5107:Rings of Uranus
5095:
5081:
5079:Moons of Uranus
5076:
5046:
5041:
5023:
5003:
4963:
4944:
4912:
4895:
4891:
4885:
4881:
4862:
4846:
4842:William Lassell
4837:James L. Elliot
4808:
4770:
4739:
4726:
4721:
4677:of Titania) at
4658:
4656:
4655:on June 4, 2011
4642:
4633:
4631:
4617:
4603:
4601:
4592:
4589:
4584:
4580:August 25, 2015
4571:
4567:
4554:
4550:
4533:
4521:
4497:
4496:
4492:
4452:
4447:
4446:
4442:
4433:
4432:
4428:
4419:
4418:
4414:
4384:
4383:
4379:
4339:
4338:
4329:
4293:
4292:
4283:
4261:
4260:
4256:
4234:
4233:
4218:
4209:
4207:
4186:
4185:
4181:
4172:
4170:
4153:
4152:
4141:
4103:
4102:
4093:
4055:
4054:
4033:
4015:
4014:
4001:
3992:
3991:
3987:
3951:
3950:
3935:
3905:
3904:
3900:
3891:
3889:
3884:
3883:
3879:
3843:
3842:
3838:
3808:
3807:
3803:
3766:(4759): 85–89.
3757:
3756:
3752:
3704:
3700:
3696:
3695:
3666:
3657:
3655:
3650:
3649:
3645:
3612:
3611:
3607:
3571:
3570:
3566:
3530:
3529:
3525:
3515:
3513:
3503:
3502:
3498:
3462:
3461:
3457:
3436:
3435:
3431:
3387:
3386:
3382:
3341:
3340:
3336:
3300:
3299:
3295:
3248:
3247:
3243:
3206:Herschel, W. S.
3204:
3203:
3199:
3192:
3177:
3176:
3169:
3136:
3135:
3126:
3089:(4759): 43–64.
3076:
3075:
3046:
3041:
3037:
2985:
2984:
2980:
2970:
2968:
2964:
2933:
2927:
2926:
2907:
2898:
2896:
2891:
2890:
2877:
2868:
2864:
2828:
2827:
2823:
2786:Herschel, W. S.
2784:
2783:
2776:
2772:
2767:
2758:
2754:
2749:
2745:
2741:
2736:
2732:
2699:
2695:
2678:
2674:
2665:
2663:
2662:
2657:and the radius
2645:
2641:
2629:and the radius
2617:
2613:
2596:
2592:
2579:
2575:
2570:
2566:
2557:
2553:
2549:
2532:
2491:One possibility
2465:
2459:
2441:ammonia hydrate
2418:
2410:
2405:carbon monoxide
2393:moons of Saturn
2381:
2365:
2335:a bright star (
2322:summer solstice
2307:
2302:
2281:
2279:
2275:
2272:
2267:
2264:
2262:
2260:
2259:
2232:
2230:
2226:
2223:
2218:
2215:
2213:
2211:
2210:
2183:
2181:
2177:
2174:
2169:
2166:
2164:
2162:
2161:
2152:Timon of Athens
2134:
2132:
2128:
2125:
2120:
2117:
2115:
2113:
2112:
2085:
2083:
2079:
2076:
2071:
2068:
2066:
2064:
2063:
2036:
2034:
2030:
2027:
2022:
2019:
2017:
2015:
2014:
1987:
1985:
1981:
1978:
1973:
1970:
1968:
1966:
1965:
1938:
1936:
1932:
1929:
1924:
1921:
1919:
1917:
1916:
1891:
1889:
1885:
1882:
1877:
1874:
1872:
1870:
1869:
1842:
1840:
1836:
1833:
1828:
1825:
1823:
1821:
1820:
1795:
1793:
1789:
1786:
1781:
1778:
1776:
1774:
1773:
1741:
1739:
1735:
1732:
1727:
1724:
1722:
1720:
1719:
1687:
1685:
1681:
1679:
1675:
1674:
1671:
1666:
1663:
1661:
1659:
1658:
1628:
1626:
1622:
1619:
1614:
1611:
1609:
1607:
1606:
1579:
1577:
1573:
1570:
1565:
1562:
1560:
1558:
1557:
1525:
1523:
1519:
1516:
1511:
1508:
1506:
1504:
1503:
1475:Rousillon Rupes
1462:
1460:
1456:
1453:
1448:
1445:
1443:
1441:
1440:
1404:
1402:
1398:
1395:
1390:
1387:
1385:
1383:
1382:
1355:Belmont Chasma
1299:Rousillon Rupes
1233:micrometeorites
1192:
1149:
1145:
1041:
985:of Uranus. Its
971:
919:
915:
884:
880:
872:
864:William Lassell
858:
843:William Lassell
790:
641:
614:
610:
600:
558:
540:
518:
486:
461:
449:
447:Escape velocity
434:
432:Surface gravity
423:1.683 g/cm
422:
419:
405:
401:
399:
385:
382:
379:
377:
363:
360:
358:
355:
343:
337:
335:
332:
303:
290:
276:
274:
271:
260:
246:
244:
241:
239:Semi-major axis
193:
189:
149:
122:
118:
107:
70:
69:at lower right.
35:
28:
23:
22:
15:
12:
11:
5:
6279:
6277:
6269:
6268:
6263:
6258:
6253:
6251:Titania (moon)
6243:
6242:
6238:
6237:
6225:
6213:
6201:
6189:
6166:
6165:
6163:
6162:
6157:
6152:
6147:
6142:
6137:
6132:
6127:
6122:
6116:
6113:
6112:
6110:
6109:
6106:
6101:
6096:
6091:
6086:
6081:
6076:
6071:
6066:
6061:
6056:
6051:
6046:
6041:
6036:
6031:
6026:
6021:
6016:
6011:
6006:
6001:
5996:
5991:
5986:
5981:
5976:
5971:
5970:
5969:
5955:
5953:
5947:
5946:
5944:
5943:
5938:
5933:
5932:
5931:
5922:Gǃkúnǁʼhòmdímà
5919:
5918:
5917:
5905:
5904:
5903:
5891:
5886:
5881:
5876:
5875:
5874:
5867:
5855:
5851:
5850:
5849:
5848:
5836:
5835:
5834:
5822:
5821:
5820:
5808:
5804:
5803:
5797:
5792:
5787:
5786:
5785:
5773:
5772:
5771:
5759:
5758:
5757:
5752:
5742:
5737:
5732:
5731:
5730:
5725:
5715:
5714:
5713:
5706:
5694:
5693:
5692:
5680:
5679:
5678:
5668:
5663:
5662:
5661:
5649:
5645:
5644:
5639:
5634:
5627:
5626:
5625:
5613:
5612:
5611:
5599:
5594:
5590:
5588:
5580:
5579:
5577:
5576:
5571:
5566:
5561:
5556:
5551:
5546:
5540:
5538:
5529:
5528:
5509:
5507:
5505:
5504:
5499:
5494:
5489:
5484:
5479:
5473:
5471:
5462:
5461:
5452:
5450:
5449:
5442:
5435:
5427:
5418:
5417:
5415:
5414:
5413:
5412:
5407:
5402:
5392:
5391:
5390:
5385:
5380:
5375:
5365:
5360:
5359:
5358:
5353:
5343:
5342:
5341:
5331:
5330:
5329:
5324:
5313:
5311:
5307:
5306:
5303:
5302:
5300:
5299:
5294:
5289:
5284:
5279:
5274:
5269:
5264:
5259:
5253:
5251:
5247:
5246:
5244:
5243:
5237:
5235:
5228:
5224:
5223:
5221:
5220:
5213:
5206:
5199:
5192:
5184:
5182:
5178:
5177:
5175:
5174:
5169:
5164:
5159:
5154:
5149:
5144:
5139:
5134:
5129:
5124:
5119:
5114:
5109:
5103:
5101:
5097:
5096:
5094:
5093:
5086:
5083:
5082:
5077:
5075:
5074:
5067:
5060:
5052:
5043:
5042:
5040:
5039:
5028:
5025:
5024:
5022:
5021:
5015:
5013:
5009:
5008:
5005:
5004:
5002:
5001:
4996:
4991:
4984:
4977:
4971:
4969:
4965:
4964:
4962:
4961:
4952:
4950:
4946:
4945:
4943:
4942:
4933:
4931:
4924:
4918:
4917:
4914:
4913:
4911:
4910:
4905:
4900:
4899:
4898:
4893:
4888:
4883:
4872:
4870:
4864:
4863:
4861:
4860:
4854:
4852:
4848:
4847:
4845:
4844:
4839:
4834:
4829:
4823:
4821:
4814:
4810:
4809:
4807:
4806:
4801:
4796:
4791:
4786:
4780:
4778:
4772:
4771:
4769:
4768:
4763:
4758:
4753:
4747:
4745:
4741:
4740:
4738:
4737:
4731:
4728:
4727:
4722:
4720:
4719:
4712:
4705:
4697:
4691:
4690:
4681:
4665:
4640:
4615:
4610:
4588:
4587:External links
4585:
4583:
4582:
4572:Stephen Clark
4565:
4563:24 August 2009
4548:
4519:
4511:10.17226/26522
4490:
4440:
4426:
4412:
4377:
4327:
4281:
4254:
4216:
4179:
4139:
4091:
4031:
3999:
3985:
3966:(1): 258–273.
3933:
3928:10.1086/116211
3898:
3877:
3856:(2): 599–602.
3836:
3817:(1): 343–346.
3801:
3750:
3713:(2): 543–555.
3702:
3698:
3664:
3643:
3638:10.1086/100198
3605:
3564:
3523:
3496:
3455:
3429:
3415:10.1086/126146
3380:
3345:(March 1834).
3343:Herschel, John
3334:
3293:
3241:
3197:
3190:
3167:
3124:
3044:
3035:
2978:
2944:(2): 458–476.
2905:
2875:
2862:
2821:
2773:
2771:
2768:
2766:
2765:
2759:For instance,
2752:
2747:
2739:
2730:
2693:
2672:
2639:
2611:
2590:
2573:
2564:
2550:
2548:
2545:
2544:
2543:
2538:
2531:
2528:
2475:Voyager 2
2461:Main article:
2458:
2455:
2416:
2408:
2385:accretion disc
2380:
2377:
2363:
2326:vapor pressure
2305:
2301:
2298:
2295:
2294:
2290:
2289:
2257:
2254:
2245:
2241:
2240:
2208:
2205:
2198:
2192:
2191:
2179:24.3°S 309.2°E
2159:
2156:
2147:
2143:
2142:
2130:11.9°S 302.2°E
2110:
2107:
2098:
2094:
2093:
2061:
2058:
2049:
2045:
2044:
2032:14.7°S 277.1°E
2012:
2009:
2000:
1996:
1995:
1983:51.2°S 331.9°E
1963:
1960:
1951:
1947:
1946:
1934:55.3°S 285.9°E
1914:
1911:
1904:
1900:
1899:
1887:19.2°S 338.8°E
1867:
1864:
1855:
1851:
1850:
1838:23.8°S 321.2°E
1818:
1815:
1808:
1804:
1803:
1791:15.8°S 287.1°E
1771:
1768:
1756:
1750:
1749:
1737:44.8°S 333.6°E
1717:
1714:
1702:
1698:
1697:
1677:42.4°S 291.4°E
1656:
1653:
1641:
1637:
1636:
1624:55.8°S 351.2°E
1604:
1601:
1592:
1588:
1587:
1555:
1552:
1547:
1538:
1534:
1533:
1501:
1498:
1493:
1477:
1471:
1470:
1438:
1435:
1419:
1413:
1412:
1380:
1377:
1372:
1356:
1352:
1351:
1348:
1345:
1342:
1339:
1295:Messina Chasma
1191:
1188:
1147:
1143:
1123:carbon dioxide
1040:
1037:
999:tidally locked
987:orbital period
970:
967:
868:Roman numerals
825:Alexander Pope
789:
786:
768:carbon dioxide
754:accretion disk
738:impact craters
677:moon of Uranus
602:
601:
599:
598:
592:
586:
583:carbon dioxide
579:
577:
571:
570:
559:
553:
550:
549:
545:
544:
541:
536:
533:
532:
529:
528:
525:
516:
513:
509:
508:
505:
502:
499:
488:
487:
485:
484:
481:
477:
475:
469:
468:
462:
457:
454:
453:
450:
445:
442:
441:
435:
430:
427:
426:
420:
414:
411:
410:
397:
391:
390:
375:
369:
368:
356:
351:
348:
347:
333:
328:
325:
324:
320:
319:
314:
308:
307:
301:
295:
294:
293:3.64 km/s
291:
285:
282:
281:
272:
267:
264:
263:
258:
252:
251:
242:
237:
234:
233:
227:
226:
186:
180:
179:
116:
112:
111:
108:
105:
102:
101:
97:
96:
93:
89:
88:
83:
77:
76:
72:
71:
50:
26:
24:
14:
13:
10:
9:
6:
4:
3:
2:
6278:
6267:
6264:
6262:
6259:
6257:
6254:
6252:
6249:
6248:
6246:
6236:
6226:
6224:
6214:
6212:
6202:
6200:
6195:
6190:
6188:
6178:
6174:
6161:
6158:
6156:
6155:Regular moons
6153:
6151:
6148:
6146:
6143:
6141:
6138:
6136:
6133:
6131:
6128:
6126:
6123:
6121:
6118:
6117:
6114:
6107:
6105:
6102:
6100:
6097:
6095:
6092:
6090:
6087:
6085:
6082:
6080:
6077:
6075:
6072:
6070:
6067:
6065:
6062:
6060:
6057:
6055:
6052:
6050:
6047:
6045:
6042:
6040:
6037:
6035:
6032:
6030:
6027:
6025:
6022:
6020:
6017:
6015:
6012:
6010:
6007:
6005:
6002:
6000:
5997:
5995:
5992:
5990:
5987:
5985:
5982:
5980:
5977:
5975:
5972:
5966:
5962:
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5356:Mommur Chasma
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4909:
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4903:83982 Crantor
4901:
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4878:
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4865:
4859:
4856:
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4853:
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4832:Gerard Kuiper
4830:
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4441:
4437:. 9 May 2023.
4436:
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4250:
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4231:
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4225:
4223:
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4217:
4206:on 2012-05-27
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3996:. 4 May 2023.
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3441:(in German).
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2876:
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2869:Lewis (2002)
2866:
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2299:
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2258:
2255:
2252:
2251:
2246:
2242:
2237:
2228:12.4°S 45.2°E
2209:
2206:
2203:
2199:
2197:
2193:
2188:
2160:
2157:
2154:
2153:
2148:
2144:
2139:
2111:
2108:
2105:
2104:
2099:
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2090:
2062:
2059:
2056:
2055:
2050:
2046:
2041:
2013:
2010:
2007:
2006:
2001:
1997:
1992:
1964:
1961:
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1952:
1948:
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1649:Julius Caesar
1645:
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1638:
1633:
1605:
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1599:
1598:
1593:
1589:
1584:
1556:
1553:
1551:
1545:
1544:
1539:
1535:
1530:
1521:14.7°S 23.5°E
1502:
1499:
1497:
1494:
1491:
1490:
1485:
1481:
1478:
1476:
1472:
1467:
1439:
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1370:
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1364:
1360:
1357:
1353:
1336:
1326:
1322:
1320:
1315:
1314:impact crater
1310:
1308:
1307:cryovolcanism
1304:
1300:
1296:
1292:
1288:
1283:
1281:
1277:
1273:
1269:
1265:
1261:
1257:
1253:
1249:
1244:
1242:
1238:
1234:
1230:
1225:
1224:Ursula crater
1221:
1217:
1213:
1209:
1205:
1196:
1189:
1187:
1184:
1180:
1176:
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1141:
1137:
1132:
1128:
1124:
1119:
1117:
1113:
1109:
1105:
1101:
1096:
1092:
1088:
1087:spectroscopic
1085:
1081:
1077:
1073:
1064:
1060:
1056:
1052:
1050:
1045:
1038:
1036:
1034:
1030:
1026:
1022:
1018:
1014:
1009:
1007:
1006:magnetosphere
1002:
1000:
996:
992:
988:
984:
980:
976:
968:
966:
964:
960:
956:
952:
946:
911:
877:
875:
869:
865:
861:
854:
852:
848:
844:
840:
836:
835:
830:
826:
822:
815:, and Titania
814:
810:
805:
801:
799:
795:
787:
785:
783:
782:
777:
773:
769:
765:
761:
757:
755:
751:
747:
743:
739:
735:
731:
727:
723:
719:
714:
712:
711:magnetosphere
708:
704:
703:
698:
694:
690:
686:
682:
678:
674:
668:
608:
596:
593:
590:
587:
584:
581:
580:
578:
576:
572:
568:
564:
561:<1–2
560:
557:
551:
546:
542:
539:
534:
526:
524:
517:
514:
511:
510:
506:
503:
500:
498:
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489:
482:
479:
478:
476:
474:
470:
467:
463:
460:
455:
451:
448:
443:
440:
436:
433:
428:
421:
418:
412:
398:
396:
392:
376:
374:
370:
357:
354:
349:
334:
331:
326:
321:
318:
315:
313:
309:
302:
300:
296:
292:
289:
288:orbital speed
283:
273:
270:
265:
259:
257:
253:
243:
240:
235:
232:
228:
223:
187:
185:
181:
176:
117:
115:Pronunciation
113:
109:
103:
98:
94:
90:
87:
84:
82:
78:
73:
68:
64:
60:
59:impact crater
56:
55:
48:
43:
37:
33:
19:
6235:Solar System
6160:Trojan moons
6150:Subsatellite
6003:
5964:
5689:Petit-Prince
5584:Minor-planet
5533:Dwarf planet
5458:Solar System
5339:Verona Rupes
5215:
5209:
5208:
5201:
5194:
5187:
4986:
4979:
4955:
4941:(1986 flyby)
4936:
4798:
4678:
4668:Titania page
4657:. Retrieved
4653:the original
4632:. Retrieved
4628:the original
4602:. Retrieved
4598:the original
4577:
4568:
4560:
4551:
4501:
4493:
4460:
4456:
4443:
4429:
4415:
4390:
4386:
4380:
4345:
4341:
4303:
4299:
4267:
4263:
4257:
4240:
4236:
4208:. Retrieved
4204:the original
4199:
4182:
4171:. Retrieved
4166:
4109:
4105:
4061:
4057:
4017:
3988:
3963:
3957:
3911:
3907:
3901:
3890:. Retrieved
3880:
3853:
3849:
3839:
3814:
3810:
3804:
3763:
3759:
3753:
3710:
3706:
3656:. Retrieved
3646:
3621:
3617:
3608:
3581:
3577:
3567:
3543:(3): 43–44.
3540:
3536:
3526:
3514:. Retrieved
3509:
3499:
3472:
3468:
3458:
3442:
3438:
3432:
3400:(360): 129.
3397:
3393:
3383:
3359:(5): 35–36.
3356:
3350:
3337:
3313:(3): 44–47.
3310:
3306:
3296:
3261:
3257:
3244:
3217:
3213:
3200:
3180:
3148:(1): 51–68.
3145:
3141:
3086:
3082:
3038:
2995:
2991:
2981:
2969:. Retrieved
2962:the original
2941:
2937:
2897:. Retrieved
2870:
2865:
2854:
2850:
2845:the original
2833:
2824:
2797:
2793:
2755:
2742:
2733:
2696:
2675:
2658:
2654:
2647:
2642:
2634:
2630:
2626:
2619:
2614:
2606:
2602:
2598:
2593:
2585:
2581:
2576:
2567:
2554:
2509:
2494:
2488:
2474:
2468:
2466:
2435:The initial
2434:
2421:
2382:
2373:carbon cycle
2360:solar energy
2357:
2330:
2303:
2277:34.5°S 4.2°E
2248:
2201:
2184:-24.3; 309.2
2150:
2135:-11.9; 302.2
2101:
2081:15.5°S 316°E
2052:
2037:-14.7; 277.1
2003:
1988:-51.2; 331.9
1954:
1939:-55.3; 285.9
1907:
1892:-19.2; 338.8
1858:
1843:-23.8; 321.2
1796:-15.8; 287.1
1762:
1742:-44.8; 333.6
1708:
1682:-42.4; 291.4
1647:
1629:-55.8; 351.2
1595:
1575:20.1°S 3.9°E
1541:
1487:
1458:33.3°S 335°E
1429:
1400:8.5°S 32.6°E
1366:
1350:Coordinates
1341:Named after
1311:
1302:
1284:
1245:
1237:Solar System
1201:
1152:
1120:
1076:carbonaceous
1068:
1047:
1033:occultations
1024:
1010:
1003:
975:eccentricity
972:
962:
954:
878:
871:
857:
855:
832:
818:
791:
779:
758:
715:
700:
685:Solar System
672:
606:
605:
565:(10–20
425:(calculated)
353:Surface area
256:Eccentricity
100:Designations
52:
36:
32:Titan (moon)
6223:Outer space
6211:Spaceflight
6125:Inner moons
5831:Skamandrios
4922:Exploration
4868:Co-orbitals
4776:Major moons
4670:(including
4306:: 373–380.
4112:(1): 1–13.
3516:25 February
3220:: 364–378.
2855:The Tempest
2800:: 125–129.
2457:Exploration
2411:instead of
2280: /
2233:-12.4; 45.2
2231: /
2182: /
2133: /
2084: /
2035: /
1986: /
1953:Katherine (
1937: /
1890: /
1841: /
1794: /
1740: /
1680: /
1640:Calphurnia
1627: /
1578: /
1526:-14.7; 23.5
1524: /
1461: /
1403: /
1216:Bond albedo
1131:ultraviolet
1091:crystalline
995:synchronous
961:. The name
724:and an icy
483:0.17 (Bond)
466:synchronous
340:0.6 km
330:Mean radius
299:Inclination
106:Designation
6245:Categories
5889:Sila–Nunam
5755:Cleoselene
5750:Alexhelios
5728:Gorgoneion
5666:Euphrosyne
5593:Near-Earth
5535:satellites
5468:satellites
5395:Umbrielian
5272:S/2023 U 1
5250:Retrograde
4751:Atmosphere
4270:: 964–65.
4210:2012-02-23
4173:2012-02-23
3892:2009-05-28
3658:2009-09-26
3624:(33): 70.
3584:(6): 135.
3510:folger.edu
3005:2401.04634
2998:: 115957.
2899:2009-10-06
2770:References
2716:, Earth's
2605: : 4π
2584: : 4π
2369:sublimates
2337:HIP 106829
2300:Atmosphere
2282:-34.5; 4.2
2250:Coriolanus
2086:-15.5; 316
1956:Henry VIII
1950:Katherine
1686: (
1580:-20.1; 3.9
1480:Roussillon
1463:-33.3; 335
1405:-8.5; 32.6
1171:antifreeze
1165:(5.8
1140:primordial
1136:outgassing
1127:carbonates
873:Uranus III
772:atmosphere
673:Uranus III
548:Atmosphere
452:0.765 km/s
408:10 kg
184:Adjectives
110:Uranus III
6187:Astronomy
6054:Enceladus
5928:Gǃòʼé ǃHú
5839:Eurybates
5817:Menoetius
5811:Patroclus
5800:Dinkinesh
5745:Kleopatra
5648:Main belt
5608:Dimorphos
5466:Planetary
5346:Oberonian
5334:Mirandian
5297:Ferdinand
5257:Francisco
5132:Desdemona
4968:Proposals
4957:Tianwen-4
4938:Voyager 2
4820:Discovery
4813:Astronomy
4761:Dark Spot
4744:Geography
4686:from the
4537:cite book
4529:248283239
4485:0148-0227
4134:0019-1035
4086:0148-0227
3720:0704.1525
3475:: 15–17.
3424:119916925
3288:186208735
3264:: 47–79.
3030:0019-1035
2830:"Titania"
2470:Voyager 2
2389:obliquity
2345:ephemeris
2339:) with a
2247:Valeria (
2149:Phrynia (
2002:Lucetta (
1906:Jessica (
1812:Cymbeline
1540:Adriana (
1057:and long
1049:Voyager 2
1025:Voyager 2
781:Voyager 2
734:endogenic
689:Australia
527:89 K
515:60 K
464:presumed
188:Titanian
75:Discovery
54:Voyager 2
6099:Hyperion
6049:Dysnomia
5979:Callisto
5959:Ganymede
5782:Olympias
5652:Kalliope
5622:Squannit
5597:Florence
5569:Gonggong
5564:Makemake
5373:Gertrude
5368:Titanian
5317:Arielian
5287:Prospero
5277:Trinculo
5267:Stephano
5241:Margaret
5234:Prograde
5147:Rosalind
5127:Cressida
5112:Cordelia
5037:Category
4672:labelled
4659:June 22,
4634:June 22,
4604:June 22,
3796:43471184
3788:17812894
3745:12105236
3701:O and CO
3111:17812889
2873:, p. 387
2788:(1787).
2710:Callisto
2702:Ganymede
2661: :
2633: :
2530:See also
2397:nitrogen
2333:occulted
2314:nitrogen
2310:Callisto
2244:Valeria
2200:Ursula (
2170:309°12′E
2146:Phrynia
2121:302°12′E
2072:316°00′E
2051:Marina (
2023:277°06′E
1999:Lucetta
1974:331°54′E
1925:285°54′E
1903:Jessica
1878:338°48′E
1829:321°12′E
1810:Imogen (
1782:287°06′E
1759:Gertrude
1754:Gertrude
1728:333°36′E
1667:291°24′E
1615:351°12′E
1537:Adriana
1449:335°00′E
1338:Feature
1319:tectonic
1268:Gertrude
1252:chasmata
1118:behind.
1084:infrared
1021:solstice
979:inclined
955:Titanian
951:titanium
859:Uranus I
760:Infrared
589:nitrogen
556:pressure
554:Surface
512:solstice
495:Surface
388: km
366: km
286:Average
249: km
63:Gertrude
6173:Portals
6089:Hiʻiaka
6069:Proteus
6059:Miranda
6029:Umbriel
6019:Iapetus
6004:Titania
5965:largest
5952:by size
5937:2013 FY
5894:Salacia
5880:2002 UX
5802:(Selam)
5790:Pulcova
5740:Elektra
5735:Camilla
5718:Minerva
5703:Romulus
5683:Eugenia
5676:Peneius
5638:2001 SN
5631:1994 CC
5602:Didymos
5502:Neptune
5487:Jupiter
5456:of the
5363:Puckian
5327:Yangoor
5292:Setebos
5282:Sycorax
5262:Caliban
5210:Titania
5203:Umbriel
5189:Miranda
5162:Perdita
5157:Belinda
5117:Ophelia
5019:Fiction
5012:Related
4981:OCEANUS
4892:2014 YX
4882:2011 QF
4876:Trojans
4851:General
4799:Titania
4794:Umbriel
4784:Miranda
4756:Climate
4735:Outline
4465:Bibcode
4395:Bibcode
4350:Bibcode
4308:Bibcode
4272:Bibcode
4245:Bibcode
4114:Bibcode
4066:Bibcode
4022:Bibcode
3968:Bibcode
3916:Bibcode
3858:Bibcode
3819:Bibcode
3768:Bibcode
3760:Science
3725:Bibcode
3626:Bibcode
3586:Bibcode
3545:Bibcode
3477:Bibcode
3447:Bibcode
3445:: 325.
3402:Bibcode
3361:Bibcode
3315:Bibcode
3266:Bibcode
3222:Bibcode
3150:Bibcode
3119:5895824
3091:Bibcode
3083:Science
3010:Bibcode
2971:June 3,
2946:Bibcode
2689:Umbriel
2681:Miranda
2664:√
2597:Volume
2496:Cassini
2413:ammonia
2318:methane
2265:34°30′S
2219:45°12′E
2216:12°24′S
2167:24°18′S
2118:11°54′S
2100:Mopsa (
2069:15°30′S
2048:Marina
2020:14°42′S
1971:51°12′S
1922:55°18′S
1875:19°12′S
1826:23°48′S
1807:Imogen
1779:15°48′S
1725:44°48′S
1701:Elinor
1664:42°24′S
1612:55°48′S
1563:20°06′S
1512:23°30′E
1509:14°42′S
1446:33°18′S
1422:Messina
1391:32°36′E
1359:Belmont
1303:Voyager
1291:grabens
1276:Jessica
1256:canyons
1248:craters
1204:Miranda
1138:of the
1116:residue
1108:methane
1104:sputter
1029:equinox
983:equator
977:and is
963:Titania
851:Umbriel
746:canyons
683:in the
607:Titania
595:methane
417:density
404:0.0509)
400:(3.4550
279: d
67:grabens
40:Titania
6145:Naming
6104:Phoebe
6094:Actaea
6084:Nereid
6079:Ilmarë
6044:Tethys
6024:Charon
6014:Oberon
5999:Triton
5994:Europa
5950:Ranked
5914:Ilmarë
5900:Actaea
5825:Hektor
5776:Roxane
5768:Dactyl
5697:Sylvia
5671:Daphne
5616:Moshup
5559:Quaoar
5554:Haumea
5497:Uranus
5492:Saturn
5383:Ursula
5351:Hamlet
5217:Oberon
5142:Portia
5137:Juliet
5122:Bianca
5091:Uranus
4988:ODINUS
4960:(2029)
4949:Future
4804:Oberon
4724:Uranus
4527:
4517:
4483:
4132:
4106:Icarus
4084:
3959:Icarus
3811:Icarus
3794:
3786:
3743:
3707:Icarus
3422:
3286:
3188:
3142:Icarus
3117:
3109:
3028:
2992:Icarus
2938:Icarus
2835:Lexico
2816:106717
2814:
2761:Tethys
2726:Triton
2724:, and
2722:Europa
2650:, the
2622:, the
2401:carbon
2349:Triton
2268:4°12′E
2196:Ursula
2097:Mopsa
1857:Iras (
1764:Hamlet
1594:Bona (
1566:3°54′E
1550:Crater
1484:France
1437:1,492
1388:8°30′S
1375:Chasma
1287:faults
1272:Ursula
1264:scarps
1258:) and
1220:Oberon
1159:mantle
1063:Ursula
1059:scarps
1023:. The
1017:zenith
811:, the
794:Oberon
750:scarps
742:Oberon
726:mantle
707:Uranus
521:
519:70 ± 7
473:Albedo
437:0.371
373:Volume
317:Uranus
304:0.340°
261:0.0011
6199:Stars
6074:Mimas
6064:Vanth
6039:Dione
6034:Ariel
5974:Titan
5908:Varda
5864:Hiisi
5858:Lempo
5845:Queta
5795:Balam
5723:Aegis
5710:Remus
5658:Linus
5586:moons
5549:Pluto
5544:Orcus
5477:Earth
5410:Skynd
5405:Vuver
5400:Wunda
5196:Ariel
5152:Cupid
5100:Inner
4789:Ariel
4766:Rings
4525:S2CID
4453:(PDF)
3792:S2CID
3741:S2CID
3715:arXiv
3420:S2CID
3284:S2CID
3115:S2CID
3000:arXiv
2965:(PDF)
2934:(PDF)
2812:JSTOR
2706:Titan
2685:Ariel
2666:2Gm/r
2560:Titan
2547:Notes
2443:) or
2407:and N
2353:Pluto
1854:Iras
1591:Bona
1496:Rupes
1426:Italy
1363:Italy
1344:Type
1260:rupes
1227:from
1055:rifts
1013:poles
969:Orbit
959:Titan
847:Ariel
809:Earth
798:Earth
497:temp.
415:Mean
336:788.4
275:8.706
6135:List
6009:Rhea
5989:Moon
5871:Paha
5854:TNOs
5574:Eris
5482:Mars
5167:Puck
4975:MUSE
4930:Past
4675:maps
4661:2009
4636:2009
4606:2009
4543:link
4515:ISBN
4481:ISSN
4188:USGS
4155:USGS
4130:ISSN
4082:ISSN
3784:PMID
3518:2024
3186:ISBN
3107:PMID
3026:ISSN
2973:2009
2718:Moon
2635:Gm/r
2609:/3.
2445:salt
2399:and
2207:135
2109:101
1770:326
1655:100
1500:402
1379:238
1280:rays
1274:and
1167:kbar
1155:core
1074:and
1072:rock
849:and
839:John
813:Moon
776:star
748:and
722:core
718:rock
567:nbar
543:13.9
504:mean
439:m/s²
395:Mass
6108:...
5762:Ida
5640:263
5172:Mab
4507:doi
4473:doi
4403:doi
4366:hdl
4358:doi
4316:doi
4304:413
4192:IAU
4159:IAU
4122:doi
4074:doi
3976:doi
3964:185
3924:doi
3912:103
3866:doi
3854:492
3827:doi
3815:200
3776:doi
3764:233
3733:doi
3711:184
3634:doi
3594:doi
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3485:doi
3410:doi
3369:doi
3323:doi
3274:doi
3230:doi
3158:doi
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2954:doi
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2802:doi
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2158:35
2060:40
2011:58
1962:75
1913:64
1866:33
1817:28
1716:74
1603:51
1554:50
1163:GPa
997:or
862:by
831:in
823:or
764:ice
709:'s
597:(?)
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563:mPa
507:max
501:min
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380:054
364:000
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