The control network of Iapetus
Identifieur interne : 001216 ( Istex/Checkpoint ); précédent : 001215; suivant : 001217The control network of Iapetus
Auteurs : Merton E. Davies [États-Unis] ; Frank Y. Katayama [États-Unis]Source :
- Icarus [ 0019-1035 ] ; 1984.
English descriptors
- Entity :
- Teeft :
- Almeric, Analytical triangulation, Approximate camera orientation matrix, Batson, Best resolution, Camera orientation angle, Cartographic coordinate, Cassini, Cassini state, Closest approach, Control network, Control point, Crater, Crater almeric, Datum, Davy, Different direction, Equatorial, Galilean satellite, Iapetus, International astronomical union, Julian century, Julian day, Katayama, Lapetus, Light spot, Longitude, Meridian, Navigation team, Obliquity, Orientation angle, Prime meridian, Rand corporation, Rotation normal, Rotational element, Spacecraft position relative, Standard earth equatorial coordinate, Standard error, Triangulation, Voyager, Voyager spacecraft.
Abstract
Abstract: A control network of the Saturnian satellite Iapetus has been established photogrammetrically from pictures taken by the two Voyager spacecraft. Coordinates of 62 control points have been computed and listed; pixel measurements of these points were made on 14 Voyager 1 and 66 Voyager 2 pictures. Some of these points are identified on the preliminary U.S. Geological Survey map of Iapetus and many are identified by name. The Voyager 1 and Voyager 2 pictures covered limited regions of the satellite's surface and contained no overlapping areas. The longitude system on Iapetus is defined by the crater Almeric; the 276° meridian passes through the center of this crater. The obliquity of Iapetus has been measured as 0°.4 ± 1°.6. The mean radius of Iapetus has been determined as 718 ± 8 km.
Url:
DOI: 10.1016/0019-1035(84)90023-X
Affiliations:
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ISTEX:A95213D55C5F8C0660BA9130C9F097007403BC8FLe document en format XML
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<term>James A. Roth</term>
<term>Janet L. Hirsch</term>
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<term>Stewart A. Collins</term>
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<term>Analytical triangulation</term>
<term>Approximate camera orientation matrix</term>
<term>Batson</term>
<term>Best resolution</term>
<term>Camera orientation angle</term>
<term>Cartographic coordinate</term>
<term>Cassini</term>
<term>Cassini state</term>
<term>Closest approach</term>
<term>Control network</term>
<term>Control point</term>
<term>Crater</term>
<term>Crater almeric</term>
<term>Datum</term>
<term>Davy</term>
<term>Different direction</term>
<term>Equatorial</term>
<term>Galilean satellite</term>
<term>Iapetus</term>
<term>International astronomical union</term>
<term>Julian century</term>
<term>Julian day</term>
<term>Katayama</term>
<term>Lapetus</term>
<term>Light spot</term>
<term>Longitude</term>
<term>Meridian</term>
<term>Navigation team</term>
<term>Obliquity</term>
<term>Orientation angle</term>
<term>Prime meridian</term>
<term>Rand corporation</term>
<term>Rotation normal</term>
<term>Rotational element</term>
<term>Spacecraft position relative</term>
<term>Standard earth equatorial coordinate</term>
<term>Standard error</term>
<term>Triangulation</term>
<term>Voyager</term>
<term>Voyager spacecraft</term>
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<front><div type="abstract" xml:lang="en">Abstract: A control network of the Saturnian satellite Iapetus has been established photogrammetrically from pictures taken by the two Voyager spacecraft. Coordinates of 62 control points have been computed and listed; pixel measurements of these points were made on 14 Voyager 1 and 66 Voyager 2 pictures. Some of these points are identified on the preliminary U.S. Geological Survey map of Iapetus and many are identified by name. The Voyager 1 and Voyager 2 pictures covered limited regions of the satellite's surface and contained no overlapping areas. The longitude system on Iapetus is defined by the crater Almeric; the 276° meridian passes through the center of this crater. The obliquity of Iapetus has been measured as 0°.4 ± 1°.6. The mean radius of Iapetus has been determined as 718 ± 8 km.</div>
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