FM Reviews - 6. 45. Users. 29. 9,2. 14. Products. 57. 6Reviews. Views. 57,0. 39,5.
EF 5. 0mm f/1. 4 USM1,1. EF 1. 7- 4. 0mm f/4. L USM1,0. 19,4. 80. EF 2. 4- 1. 05mm f/4. L IS .. 9. 44,1. 97.
EF 2. 4- 7. 0mm f/2. L US.. 9. 29,7. 17. EF 7. 0- 2. 00mm f/4. L USM8. 43,2. 11. EF 7. 0- 2. 00mm f/2. L I.. 7. 63,6. 73. EF 1. 00- 4. 00mm f/4.
EF 7. 0- 3. 00mm f/4- 5. EF- S 1. 7- 8. 5mm f. EX APO.. 5. 72,6. EF 1. 35mm f/2. L USM5.
EF 5. 0mm f/1. 8 II5. EF- S 1. 7- 5. 5 f/2. IS .. 5. 54,9. 64.
EF 2. 8- 1. 35mm f/3. EF 3. 5mm f/1. 4. L USM5. 14,3. 53. EF 8. 5mm f/1. 8 USM5.
EF- S 1. 0- 2. 2mm f/3. EF 1. 00mm f/2. 8 Macro.. EX Asph.. 4. 50,4. EF 7. 0- 2. 00mm f/4. L IS .. 4. 45,3. 71. EF 7. 0- 2. 00mm f/2.
L U.. 4. 18,1. 20. F/2. 8 XR Di .. 4.
Miranda Kerr: Miranda Kerr in 2012: Volledige naam: Miranda May Kerr: Geboren: Sydney, 20 april 1983: Land: Australi
Miranda (moon) - Wikipedia. Miranda or Uranus V is the smallest and innermost of Uranus's five round satellites.
Like the other large moons of Uranus, Miranda orbits close to its planet's equatorial plane. Because Uranus orbits the Sun on its side, Miranda's orbit is perpendicular to the ecliptic and shares Uranus's extreme seasonal cycle. At just 4. 70 km in diameter, Miranda is one of the smallest objects in the Solar System known to be spherical under its own gravity.
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- 1eros Juegos Deportivos Internos CCPMiranda 2016: 1eros Juegos Deportivos Internos CCPMiranda 2016.
- Miranda; Discovery; Discovered by: Gerard P. Kuiper: Discovery date: February 16, 1948: Designations; Pronunciation / m .
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Of the bodies that are known to be in hydrostatic equilibrium, only Saturn's moon Mimas is smaller. Miranda has one of the most extreme and varied topographies of any object in the Solar System, including Verona Rupes, a 5- to 1. Solar System, and chevron- shaped tectonic features called coronae.
The origin and evolution of this varied geology, the most of any Uranian satellite, are still not fully understood, and multiple hypotheses exist regarding Miranda's formation. Miranda was discovered by Gerard Kuiper on 1. February 1. 94. 8 at Mc.
Donald Observatory, and named after Miranda from William Shakespeare's play The Tempest. During the flyby Miranda's southern hemisphere pointed towards the Sun, so only that part was studied. Discovery and name. Kuiper elected to name the object . However, the previous moons had been named specifically after fairies.
Subsequently discovered satellites of Uranus were named after Shakespearean characters, whether fairies or not. Of Uranus's five round satellites, Miranda orbits closest to it, at roughly 1.
Its orbital period is just 3. Moon, is synchronous with its rotation period, which means it always shows the same face to Uranus, a condition known as tidal lock. Miranda's orbital inclination (4. The reason for this is still uncertain; there are no mean- motion resonances between the moons that could explain it, leading to the hypothesis that the moons occasionally pass through secondary resonances, which at some point in the past led to Miranda being locked for a time into a 3: 1 resonance with Umbriel, before chaotic behaviour induced by the secondary resonances moved it out of it again.
That density suggests a composition of more than 6. It also has the largest known cliff in the Solar System, Verona Rupes, which has a drop- off of over 5 km (3.
Some of Miranda's terrain is possibly less than 1. Miranda may still be geologically active today. The canyons probably represent graben formed by extensional faulting. Other features may be due to cryovolcanic eruptions of icy magma. The diapirs may have changed the density distribution within Miranda, which could have caused Miranda to reorient itself. However, the maximum heating attributable to the resonance with Umbriel was likely about three times greater. Bibcode: 1. 98. 8Icar..
T. The Astronomical Journal. Bibcode: 1. 99. 2AJ.. J. M.; Kunde, V.; Maguire, W.; Pearl, J.; Pirraglia, J.; Samuelson, R.; Cruikshank, D. Bibcode: 1. 98. 6Sci.. H. JPL (Solar System Dynamics). P., The Fifth Satellite of Uranus, Publications of the Astronomical Society of the Pacific, Vol.
Mac. Donald Observatory. Celestial Mechanics and Dynamical Astronomy. Bibcode: 1. 99. 4Ce. MDA. 5. 9. 1. 29. M. An explanation of the anomalously high orbital inclination of Miranda. Bibcode: 1. 98. 9Icar..
T. Bibcode: 1. 99. Icar.. 8. 5. 4. 44. M. Archived from the original on July 9, 2.
Bibcode: 1. 98. 6Sci.. S. Journal of Geophysical Research.
Bibcode: 1. 99. 7JGR.. P. Retrieved November 2. In Lunar and Planetary Inst., Twenty- Fourth Lunar and Planetary Science Conference. Evolution through the Miranda- Umbriel 3: 1, Miranda- Ariel 5: 3, and Ariel- Umbriel 2: 1 mean- motion commensurabilities.
Bibcode: 1. 99. 0Icar.. T. The University of Michigan.