Add to ORKGThe 11 papers in this issue, comprising the Mariner 10 imaging team final report, are brought together, and the salient results of the Mariner 10 imaging experiment at Mercury are summarized. Those aspects of the data set acquired which were worked by the team are identified, and other areas where further work is needed are designated
The second Mercury encounter has resulted in the acquisition of about 360 pictures of the south pola...
Planet Mercury is both difficult to observe and difficult to reach by spacecraft. Just one spacecraf...
Volcanic and tectonic implications of the surface morphology of Mercury are discussed. Mercurian sca...
The morphology and optical properties of the surface of Mercury resemble that of the moon in remarka...
The Mariner 10 television science subsystem was an improved version of the Mariner 9 system, using 1...
More than 60,000 images of Mercury were taken at ∼29° elevation during two sunrises, at 820 nm, and ...
of the terrestrial planetary bodies, to be an exciting laboratory for the study of Solar System geol...
Prior to the flight of the Mariner 10 spacecraft, Mercury was the least investigated and most poorly...
Mariner 10 mission objectives to investigate Mercury and Venus are discussed along with the spacecra...
A preliminary geological analysis of the Mariner 10 orange/UV color ratio map of Mercury is given, a...
Mercury has a heavily cratered surface containing basins up to at least 1300 kilometers diameter flo...
Mariner 10 provided our first closeup reconnaissance of Mercury during its three flybys in 1974 and ...
A working hypothesis of Mercury's history is presented. We infer the surface of Mercury to record a ...
Prior to the return of data from the NASA MErcury Surface, Space ENvironment, GEochemistry, and Rang...
The objectives and rationale for scientific investigation of Mercury are explored. Knowledge already...
The second Mercury encounter has resulted in the acquisition of about 360 pictures of the south pola...
Planet Mercury is both difficult to observe and difficult to reach by spacecraft. Just one spacecraf...
Volcanic and tectonic implications of the surface morphology of Mercury are discussed. Mercurian sca...
The morphology and optical properties of the surface of Mercury resemble that of the moon in remarka...
The Mariner 10 television science subsystem was an improved version of the Mariner 9 system, using 1...
More than 60,000 images of Mercury were taken at ∼29° elevation during two sunrises, at 820 nm, and ...
of the terrestrial planetary bodies, to be an exciting laboratory for the study of Solar System geol...
Prior to the flight of the Mariner 10 spacecraft, Mercury was the least investigated and most poorly...
Mariner 10 mission objectives to investigate Mercury and Venus are discussed along with the spacecra...
A preliminary geological analysis of the Mariner 10 orange/UV color ratio map of Mercury is given, a...
Mercury has a heavily cratered surface containing basins up to at least 1300 kilometers diameter flo...
Mariner 10 provided our first closeup reconnaissance of Mercury during its three flybys in 1974 and ...
A working hypothesis of Mercury's history is presented. We infer the surface of Mercury to record a ...
Prior to the return of data from the NASA MErcury Surface, Space ENvironment, GEochemistry, and Rang...
The objectives and rationale for scientific investigation of Mercury are explored. Knowledge already...
The second Mercury encounter has resulted in the acquisition of about 360 pictures of the south pola...
Planet Mercury is both difficult to observe and difficult to reach by spacecraft. Just one spacecraf...
Volcanic and tectonic implications of the surface morphology of Mercury are discussed. Mercurian sca...