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Megaclite
Megaclite-Jewitt-CFHT-annotated.gif
Megaclite imaged by the Canada-France-Hawaii Telescope in December 2001
Discovery 
Discovered by Scott S. Sheppard
David C. Jewitt
Yanga R. Fernandez
Eugene A. Magnier
Discovery site Mauna Kea Observatory
Discovery date 25 November 2000
Designations
MPC designation Jupiter XIX
Pronunciation /mɛɡəˈklt/
Named after
Μεγακλειτή Megaclītē
S/2000 J 8
Adjectives Megaclitean /ˌmɛɡəklɪˈtən/
Orbital characteristics 
Epoch 27 April 2019 (JD 2458600.5)
Observation arc 16.26 yr (5,938 days)
0.1586666 AU (23,736,190 km)
Eccentricity 0.4102170
–747.09 d
269.64681°
Mean motion
0° 28m 54.732s / day
Inclination 143.20224° (to ecliptic)
356.52408°
8.71854°
Satellite of Jupiter
Physical characteristics
Mean diameter
≈ 6 km
Albedo 0.04 (assumed)
21.7
15.0

Megaclite (pronounced meh-guh-KLY-tee), also known as Jupiter XIX, is one of the many natural satellites, or moons, that orbit the giant planet Jupiter. It was first spotted by a team of astronomers from the University of Hawaii. This team was led by Scott S. Sheppard in the year 2000. When it was first found, it was given a temporary name: S/2000 J 8.

Discovering Megaclite

Megaclite was discovered on November 25, 2000. The team of astronomers included Scott S. Sheppard, David C. Jewitt, Yanga R. Fernandez, and Eugene A. Magnier. They found this moon using telescopes at the Mauna Kea Observatory in Hawaii.

Megaclite's Orbit and Size

Megaclite is a small moon, only about 6 kilometers (about 3.7 miles) wide. It travels around Jupiter at a very far distance. On average, it is about 24,687,000 kilometers (about 15.3 million miles) away from Jupiter.

It takes Megaclite about 747 days to complete one full orbit around Jupiter. This is a little over two Earth years. Megaclite's orbit is also unusual because it moves in a "retrograde" direction. This means it orbits Jupiter in the opposite direction to Jupiter's rotation. Its orbit is also quite tilted, at about 150 degrees compared to the ecliptic (the path the Sun appears to take across the sky). The orbit is also not a perfect circle; it is more of an oval shape, which scientists call having an "eccentricity" of 0.308.

Naming Megaclite

After its discovery, Megaclite was given its official name in October 2002. It was named after Megaclite, a figure from Greek mythology. In these ancient stories, Megaclite was said to be the mother of Thebe and Locrus, and her partner was Zeus. Zeus is the Greek god who is similar to the Roman god Jupiter, which is why the moon is named after her.

Megaclite's Family: The Pasiphae Group

Megaclite is part of a group of moons called the Pasiphae group. These are all irregular moons that orbit Jupiter. They are called "irregular" because their orbits are not neat and circular like some of Jupiter's larger moons.

  • Moons in the Pasiphae group orbit Jupiter at distances between 22.8 and 24.7 million kilometers.
  • Their orbits are also tilted, with inclinations ranging from 144.5 to 158.3 degrees.
  • All moons in this group, including Megaclite, have retrograde orbits.

While many moons in this group, like Pasiphae itself, appear gray, Megaclite has a light red color. This makes it look more similar to another moon called Callirrhoe.

Animation of Megaclite's orbit from 1900 to 2100
Polar view
Equatorial view
       Jupiter ·       Megaclite

See also

Kids robot.svg In Spanish: Megaclite (satélite) para niños

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