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Peale, S. J.

Publications and source records attributed to Peale, S. J..

66 records · Page 4
All sourcesNASA NTRSDOE OSTI
NASA NTRS1973

Water and the Martian W cloud.

The diurnal brightening of the W cloud region of Mars during the flyby of Mariners 6 and 7 is likely due to the formation of water ice clouds. The water required in the cloud and as vapor in the atmosphere to produce the observed brightening is estimated to be roughly between 0.1 and 10 microns. Either a qualified local source with this daily production over the W cloud area or a more probable daily uplift and saturation of existing atmosphere are compatible with observations.

Peale, S. J.↗
NASA NTRS1972

Determination of parameters related to the interior of Mercury.

Discussion of the determination possibilities and requirements for certain crucial inertia-moment and radial-mass-distribution parameters of Mercury. It is shown that the high precision of 1 min of arc, which reasonable bounds on some of these parameters demand, cannot be obtained by either earth-based observations or the television imagery of the Mariner 73 flyby. Some methods are proposed for both landers and orbiters that could determine unambiguously most of these parameters.

Peale, S. J.↗
NASA NTRS1972

The gravitational fields of the major planets

The constraints placed on models of the interiors of the major planets by the nonspherical components of their gravitational fields are explained, and several methods of determining these nonspherical components are described and evaluated.

Peale, S. J.↗
NASA NTRS1972

Determination of parameters related to the interior of Mercury

Bounds on (C-A)/C for Mercury as a function of the uncertainty in the value of the obliquity are determined. The high precision of 1 min of arc which is required for reasonable bounds on (C-A)/C cannot be obtained by either earth based observations or the television imagery of the Mariner 73 flyby. Among other methods discussed, one involving both landers and orbiters could determine unambiguously not only (C-A)/C but also (B-A)/C and C/sq MR.

Peale, S. J.↗
NASA NTRS1972

Some effects of elasticity on lunar rotation

A general Hamiltonian function for a rotating moon in the field of the earth is expanded in terms of parameters orienting the spin angular momentum relative to the principal axes of the moon and relative to coordinate axes fixed in the orbit plane. The effects of elastic distortion are included as modifications of the moment of inertia tensor, where the magnitude of the distortion is parameterized by the Love number k sub 2.

Peale, S. J.↗
NASA NTRS1970

The obliquity of Venus

Venus obliquity dynamic implications, developing equations for independent parameter set to define spin vector

Goldreich, P.↗
NASA NTRS1969

Generalized Cassini's laws.

Cassini laws applied to moon and Mercury, determining relations between moment differences for spin vector, orbital angular-momentum vector and precessional velocity

Peale, S. J.↗
NASA NTRS1968

Lunar rivers.

Lunar sinuous rills origin, suggesting surface erosion by water rivers released from permafrost ice cover during meteoritic impact

Lingenfelter, R. E.↗