Mostrando entradas con la etiqueta Ganymede. Mostrar todas las entradas
Mostrando entradas con la etiqueta Ganymede. Mostrar todas las entradas

miércoles, 12 de febrero de 2014

NASA : NASA Awards Information Technology Contract

Largest Solar System Moon Detailed in Geologic Map

Youtube Override:
Animation of a rotating globe of Jupiter's moon Ganymede, with a geologic map superimposed over a global color mosaic. The 37-second animation begins as a global color mosaic image of the moon then quickly fades in the geologic map.
Image Credit:
USGS Astrogeology Science Ctr/Wheaton/ASU/NASA/JPL-Caltech
Ganymede global geologic map
To present the best information in a single view of Jupiter's moon Ganymede, a global image mosaic was assembled, incorporating the best available imagery from NASA's Voyager 1 and 2 spacecraft and NASA's Galileo spacecraft.
Image Credit:
USGS Astrogeology Science Center/Wheaton/NASA/JPL-Caltech

More than 400 years after its discovery by astronomer Galileo Galilei, the largest moon in the solar system – Jupiter's moon Ganymede – has finally claimed a spot on the map.
A group of scientists led by Geoffrey Collins of Wheaton College has produced the first global geologic map of Ganymede, Jupiter’s seventh moon. The map combines the best images obtained during flybys conducted by NASA's Voyager 1 and 2 spacecraft (1979) and Galileo orbiter (1995 to 2003) and is now published by the U. S. Geological Survey as a global map. It technically illustrates the varied geologic character of Ganymede’s surface and is the first global, geologic map of this icy, outer-planet moon.
“This map illustrates the incredible variety of geological features on Ganymede and helps to make order from the apparent chaos of its complex surface,” said Robert Pappalardo of NASA’s Jet Propulsion Laboratory in Pasadena, Calif. “This map is helping planetary scientists to decipher the evolution of this icy world and will aid in upcoming spacecraft observations.”
The European Space Agency's Jupiter Icy Moons Explorer mission is slated to be orbiting Ganymede around 2032. NASA is contributing a U.S.-led instrument and hardware for two European-led instruments for the mission.
Since its discovery in January 1610, Ganymede has been the focus of repeated observation, first by Earth-based telescopes, and later by the flyby missions and spacecraft orbiting Jupiter. These studies depict a complex, icy world whose surface is characterized by the striking contrast between its two major terrain types: the dark, very old, highly cratered regions, and the lighter, somewhat younger (but still very old) regions marked with an extensive array of grooves and ridges.
According to the scientists who have constructed this map, three major geologic periods have been identified for Ganymede that involve the dominance of impact cratering, then tectonic upheaval, followed by a decline in geologic activity. The map, which illustrates surface features, such as furrows, grooves and impact craters, allows scientists to decipher distinct geologic time periods for an object in the outer solar system for the first time.
“The highly detailed, colorful map confirmed a number of outstanding scientific hypotheses regarding Ganymede’s geologic history, and also disproved others,” said Baerbel Lucchitta, scientist emeritus at the U.S. Geological Survey in Flagstaff, Ariz., who has been involved with geologic mapping of Ganymede since 1980. “For example, the more detailed Galileo images showed that cryovolcanism, or the creation of volcanoes that erupt water and ice, is very rare on Ganymede.”
The Ganymede global geologic map will enable researchers to compare the geologic characters of other icy satellite moons, because almost any type of feature that is found on other icy satellites has a similar feature somewhere on Ganymede.
“The surface of Ganymede is more than half as large as all the land area on Earth, so there is a wide diversity of locations to choose from,” Collins said. Ganymede also shows features that are ancient alongside much more recently formed features, adding historical diversity in addition to geographic diversity.”
Amateur astronomers can observe Ganymede (with binoculars) in the evening sky this month, as Jupiter is in opposition and easily visible.
The project was funded by NASA through its Outer Planets Research and Planetary Geology and Geophysics Programs. NASA's Jet Propulsion Laboratory is managed by the California Institute of Technology, Pasadena.
NASA
Guillermo Gonzalo Sánchez Achutegui

domingo, 24 de febrero de 2013

ESA - ESA chooses instruments for its Jupiter icy moons explorer


JUICE
21 February 2013
The JUpiter ICy moons Explorer mission, JUICE, will carry a total of 11 scientific experiments to study the gas giant planet and its large ocean-bearing moons, ESA announced today.
JUICE is the first Large-class mission in ESA’s Cosmic Vision 2015–2025 programme. Planned for launch in 2022 and arrival at Jupiter in 2030, it will spend at least three years making detailed observations of the biggest planet in the Solar System and three of its largest moons, Ganymede, Callisto and Europa.
These moons are thought to harbour vast water oceans beneath their icy surfaces and JUICE will map their surfaces, sound their interiors and assess their potential for hosting life in their oceans.
Today, ESA’s Science Programme Committee approved a complement of instruments that includes cameras and spectrometers, a laser altimeter and an ice-penetrating radar. The mission will also carry a magnetometer, plasma and particle monitors, and radio science hardware.
The instruments will be developed by scientific teams from 15 European countries, the US and Japan, through corresponding national funding.
“The selection of JUICE’s instruments is a key milestone in ESA’s flagship mission to the outer Solar System, which represents an unprecedented opportunity to showcase leading European technological and scientific expertise,” says Alvaro Giménez Cañete, ESA’s Director of Science and Robotic Exploration.
“The suite of instruments addresses all of the mission’s science goals, from in-situ measurements of Jupiter’s vast magnetic field and plasma environment, to remote observations of the surfaces and interiors of the three icy moons,” adds Luigi Colangeli, coordinator of ESA’s Solar System Missions.
Throughout its mission, JUICE will observe Jupiter’s atmosphere and magnetosphere, and the interaction of all four Galilean satellites – the three icy moons plus Io – with the gas giant planet.
The spacecraft will perform a dozen flybys of Callisto, the most heavily cratered object in the Solar System, and will fly past Europa twice in order to make the first measurements of the thickness of its icy crust.
JUICE will end up in orbit around Ganymede, where it will study the moon’s icy surface and internal structure, including its subsurface ocean.
The largest moon in the Solar System, Ganymede is the only one known to generate its own magnetic field, and JUICE will observe the unique magnetic and plasma interactions with Jupiter’s magnetosphere in detail.
“Jupiter and its icy moons constitute a kind of mini-Solar System in their own right, offering European scientists and our international partners the chance to learn more about the formation of potentially habitable worlds around other stars,” says Dmitrij Titov, ESA’s JUICE Study Scientist.
The selection of the instruments today helps to ensure that JUICE remains on schedule for launch in 2022.
List of selected experiments:
JANUS: Jovis, Amorum ac Natorum Undique Scrutator, camera system
MAJIS: Moons and Jupiter Imaging Spectrometer
UVS: UV Imaging Spectrograph
SWI: Sub-millimetre Wave Instrument
GALA: Ganymede Laser Altimeter
RIME: Radar for Icy Moons Exploration
J-MAG: Magnetometer for JUICE
PEP: Particle Environment Package
RPWI: Radio & Plasma Wave Investigation
3GM: Gravity & Geophysics of Jupiter and Galilean Moons
PRIDE: Planetary Radio Interferometer & Doppler Experiment (note this does not include spacecraft hardware but will exploit VLBI – Very Large Base Interferometry – to conduct radio science)
 
For further information, please contact:
Markus Bauer

ESA Science and Robotic Exploration Communication Officer

Tel: +31 71 565 6799

Mob: +31 61 594 3 954

Email: markus.bauer@esa.int
Luigi Colangeli
Head of ESA’s Solar System Missions Division and Coordinator of Solar System Missions
Email: luigi.colangeli@esa.int
Dmitrij Titov
ESA’s JUICE Study Scientist
Email: dmitri.titov@esa.int

ESA
Guillermo Gonzalo Sánchez Achutegui
ayabaca@gmail.com
ayabaca@hotmail.com
ayabaca@yahoo.com