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Collection:
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NASA Solarsystem Collection
Collection
NASA Solarsystem Collection
Collection
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title:
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Asteroid Ida
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description:
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This view of the asteroid 243 Ida is a mosaic of five image frames acquired by the Galileo spacecraft's solid-state imaging system at ranges of 3,057 to 3,821 kilometers (1900 to 2375 miles) on August 28, 1993, about 3.5 minutes before the spacecraft made its closest approach to the asteroid. Galileo flew about 2400 kilometers (1,500 miles) from Ida at a relative velocity of 12.4 kilometers per sec (28,000 miles per hour). Asteroid and spacecraft were 441 million kilometers (274 million miles) from the Sun. Ida is the second asteroid ever encountered by a spacecraft. It appears to be about 52 kilometers (32 miles) in length, more than twice as large as Gaspra, the first asteroid observed by Galileo in October 1991.
Ida is an irregularly shaped asteroid placed by scientists in the S class (believed to be like stony or stony iron meteorites). It is a member of the Koronis family, presumed fragments left from the breakup of a precursor asteroid in a catastrophic collision. This view shows numerous craters, including many degraded craters larger than any seen on Gaspra. The extensive cratering seems to dispel theories about Ida's surface being geologically youthful. This view also seems to rule out the idea that Ida is a double body. The south pole is believed to be in the dark side near the middle of the asteroid.
The camera's clear filter was used to produce this extremely sharp picture. Spatial resolution is 31 to 38 meters (roughly 100 feet) per pixel. A 30-frame mosaic was taken to assure capturing Ida; its position was somewhat uncertain before the Galileo encounter. Galileo shuttered and recorded a total of 150 images in order to capture Ida 21 different times during a five-hour period (about one rotation of the asteroid). Color filters were used at many of these times to allow reconstruction of color images. The Galileo project, whose primary mission was the exploration of the Jupiter system, WAs managed for NASA's Office of Space Science by the Jet Propulsion Laboratory.
*Image Credit*: NASA, Jet Propulsion Laboratory
description
This view of the asteroid 243 Ida is a mosaic of five image frames acquired by the Galileo spacecraft's solid-state imaging system at ranges of 3,057 to 3,821 kilometers (1900 to 2375 miles) on August 28, 1993, about 3.5 minutes before the spacecraft made its closest approach to the asteroid. Galileo flew about 2400 kilometers (1,500 miles) from Ida at a relative velocity of 12.4 kilometers per sec (28,000 miles per hour). Asteroid and spacecraft were 441 million kilometers (274 million miles) from the Sun. Ida is the second asteroid ever encountered by a spacecraft. It appears to be about 52 kilometers (32 miles) in length, more than twice as large as Gaspra, the first asteroid observed by Galileo in October 1991.
Ida is an irregularly shaped asteroid placed by scientists in the S class (believed to be like stony or stony iron meteorites). It is a member of the Koronis family, presumed fragments left from the breakup of a precursor asteroid in a catastrophic collision. This view shows numerous craters, including many degraded craters larger than any seen on Gaspra. The extensive cratering seems to dispel theories about Ida's surface being geologically youthful. This view also seems to rule out the idea that Ida is a double body. The south pole is believed to be in the dark side near the middle of the asteroid.
The camera's clear filter was used to produce this extremely sharp picture. Spatial resolution is 31 to 38 meters (roughly 100 feet) per pixel. A 30-frame mosaic was taken to assure capturing Ida; its position was somewhat uncertain before the Galileo encounter. Galileo shuttered and recorded a total of 150 images in order to capture Ida 21 different times during a five-hour period (about one rotation of the asteroid). Color filters were used at many of these times to allow reconstruction of color images. The Galileo project, whose primary mission was the exploration of the Jupiter system, WAs managed for NASA's Office of Space Science by the Jet Propulsion Laboratory.
*Image Credit*: NASA, Jet Propulsion Laboratory
description
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date:
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08.28.1993
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keywords:
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Solar System Exploration
keywords
Solar System Exploration
keywords
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keywords:
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SSE
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keywords:
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Space
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keywords:
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NASA
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keywords:
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National Aeronautics and Space Administration
keywords
National Aeronautics and Space Administration
keywords
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keywords:
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JPL
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keywords:
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Jet Propulsion Laboratory
keywords
Jet Propulsion Laboratory
keywords
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keywords:
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Planets
keywords
Planets
keywords
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facet_what:
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Sun
facet_what
Sun
facet_what
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facet_what:
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Galileo
facet_what
Galileo
facet_what
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facet_what:
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Jupiter
facet_what
Jupiter
facet_what
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facet_what:
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Solid-State Imaging
facet_what
Solid-State Imaging
facet_what
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facet_what:
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Asteroid Ida
facet_what
Asteroid Ida
facet_what
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facet_where:
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Jet Propulsion Laboratory
facet_where
Jet Propulsion Laboratory
facet_where
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facet_where:
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Jupiter
facet_where
Jupiter
facet_where
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facet_where:
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Jet Propulsion Laboratory (JPL)
facet_where
Jet Propulsion Laboratory (JPL)
facet_where
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facet_when:
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August 28, 1993
facet_when
August 28, 1993
facet_when
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facet_when:
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October 1991
facet_when
October 1991
facet_when
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facet_when:
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08-28-1993
facet_when
08-28-1993
facet_when
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facet_when_year:
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1991
facet_when_year
1991
facet_when_year
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facet_when_year:
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1993
facet_when_year
1993
facet_when_year
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UID:
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SPD-SLRSY-886
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original url:
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original_url
original url
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