Galileo images of Amalthea
|Discovered by||E. E. Barnard|
|Discovery date||September 9, 1892|
Mean orbit radius
|181365.84 ± 0.02 km (2.54 RJ)|
|Eccentricity||0.00319 ± 0.00004|
|0.49817943 ± 0.00000007 d (11 h 57 min 23 s)|
Average orbital speed
|Inclination||0.374 ± 0.002° (to Jupiter's equator)|
|83.5 ± 2.0 km|
|Volume||(2.43 ± 0.22)×106 km³|
|Mass||2.08 ± 0.15×1018 kg|
|0.857 ± 0.099 g/cm³|
|~0.020 m/s² (~0.002 g)|
|Albedo||0.090 ± 0.005|
On Amalthea, Jupiter would be an amazing sight in its sky, looking 92 times bigger than the Full Moon. Amalthea is the biggest of the closer moons of Jupiter. Non-spherical and reddish in colour, it is thought to have of water ice with unknown amounts of other materials. Its surface has big craters and high mountains.
Discovery and namingEdit
Amalthea was found on September 9, 1892 by Edward Emerson Barnard using the 36 inch (91 cm) telescope at Lick Observatory. It was the first new moon of Jupiter since Galileo Galilei's discovery of the Galilean moons in 1610.
The moon is named after the nymph Amalthea from Greek mythology who nursed the infant Zeus (the Greek equivalent of Jupiter) with goat's milk. Its Roman numeral designation is Jupiter V. The name "Amalthea" was not adopted by the IAU until 1975, although it had been in use for many decades. The name was suggested by Camille Flammarion. Before 1975, Amalthea was most commonly known simply as Jupiter V. The adjectival form of the name is Amalthean.
The surface of Amalthea is very red  The reddish color may be due to sulfur coming from Io or some other non ice material. Bright patches of green appear on the major slopes of Amalthea, but the nature of this color is currently unknown. The surface of Amalthea is a bit brighter than surfaces of other closer moons of Jupiter.
How Amalthea looks from JupiterEdit
How Jupiter looks from AmaltheaEdit
From the surface of Amalthea, Jupiter would look enormous: it would look 92 times bigger than the Full Moon.
In 1979-1980, the Voyager 1 and 2 spacecraft made the first images of Amalthea, which resolved its surface. They also measured the moon's surface temperature. Later, the Galileo orbiter completed taking pictures of Amalthea's surface and a close flyby enabled it to constrain the moon's internal structure and composition.
- Calculated on the basis of other parameters
- Cooper, N.J. (2006). "Cassini ISS astrometric observations of the inner jovian satellites, Amalthea and Thebe". ICARUS. 181: 223–234. doi:10.1016/j.icarus.2005.11.007. Unknown parameter
- Thomas, P.C. (1998). "The Small Inner Satellites of Jupiter". ICARUS. 135: 360–371. doi:10.1006/icar.1998.5976. Archived from the original on 2011-02-12. Retrieved 2007-12-07. Unknown parameter
- Anderson, J.D. (2005). "Amalthea's Density Is Less Than That of Water". Science. 308: 1291–1293. doi:10.1126/science.1110422. Archived from the original on 2007-06-28. Retrieved 2007-12-07. Unknown parameter
- Simonelli, D.P. (2000). "Leading/Trailing Albedo Asymmetries of Thebe, Amalthea, and Metis". ICARUS. 147: 353–365. doi:10.1006/icar.2000.6474. Archived from the original on 2007-06-28. Retrieved 2007-12-07. Unknown parameter
- Simonelli, D.P. (1982). "Amalthea: Implications of the temperature observed by Voyager". ICARUS. 54: 524–538. doi:10.1016/0019-1035(83)90244-0.
- "Classic Satellites of the Solar System". Observatorio ARVAL. Archived from the original on 2011-08-25. Retrieved 2007-09-28.
- Barnard, E. E. (1892). "Discovery and Observation of a Fifth Satellite to Jupiter". Astronomical Journal. 12: 81–85.
- IAUC 2846: Satellites of Jupiter1975 October 7. Archived 2020-06-02 at the Wayback Machine
- USGS Astrogeology Research Program, Gazetteer of Planetary Nomenclature. Archived 2007-07-26 at WebCite
- Amalthea Profile by NASA's Solar System Exploration
- Another find for Galileo – Galileo Millennium Mission status report (2003-04-09)
- Jupiter's Amalthea Surprisingly Jumbled – JPL press release (2002-12-09)
- Jupiter From Amalthea, a painting by Frank Hettick, 2002.