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Dive into the research topics where Michael E. Ash is active.

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Featured researches published by Michael E. Ash.


Science | 1968

The Case for the Radar Radius of Venus

Michael E. Ash; D. B. Campbell; R. B. Dyce; Richard P. Ingalls; R. Jurgens; Gordon H. Pettengill; Irwin I. Shapiro; M. A. Slade; T. W. Thompson

The Venus radius of 6085 � 10 kilometers, deduced from combining observations made with the Venera 4 and Mariner V space probes is incompatible with the value of 6050 � kilometers determined from Earth-based radar mesurements.


Icarus | 1969

Radar observations of Icarus

Gordon H. Pettengill; Irwin I. Shapiro; Michael E. Ash; Richard P. Ingalls; L.P. Rainville; William B. Smith; M.L. Stone

Abstract The minor planet Icarus was observed with the 3.8-cm Haystack radar from 12 to 15 June 1968. Weak but significant echoes were detected indicating a radar cross section of about 0.1 km2, a radius of about 1 km, and an effective reflectivity of about 0.05. These results have an uncertainty of about a factor of 2.


Celestial Mechanics and Dynamical Astronomy | 1976

Doubly averaged effect of the Moon and Sun on a high altitude Earth satellite orbit

Michael E. Ash

Infinite series expansions are obtained for the doubly averaged effects of the Moon and Sun on a high altitude Earth satellite, and the results used to interpret numerically integrated examples. New in this paper are: (1) both sublunar and translunar satellites are considered; (2) analytic expansions include all powers in the satellite and perturbing body semi-major axes; (3) the fact that retrograde orbits have more benign eccentricity behavior than direct orbits should be exploited for high altitude satellite systems; and (4) near circular orbits can be maintained with small expenditures of fuel in the face of an exponential driving force one forIa<I<Ib, whereIb=180°−Ia andIa is somewhat less than 39.2° for sublunar orbits and somewhat greater than 39.2° for translunar orbits.


Physical Review Letters | 1971

Fourth Test of General Relativity: New Radar Result

I. I. Shapiro; Michael E. Ash; Richard P. Ingalls


The Astronomical Journal | 1967

Astronomical constants and planetary ephemerides deduced from radar and optical observations

Michael E. Ash; I. I. Shapiro; William B. Smith


Physical Review Letters | 1968

Fourth Test of General Relativity: Preliminary Results

I. I. Shapiro; Gordon H. Pettengill; Michael E. Ash; Melvin L. Stone; William B. Smith; Richard P. Ingalls; Richard A. Brockelman


Science | 1971

The System of Planetary Masses

Michael E. Ash; I. I. Shapiro; William B. Smith


Physical Review Letters | 1972

Mercury's perihelion advance - Determination by radar.

I. I. Shapiro; Gordon H. Pettengill; Michael E. Ash; Richard P. Ingalls; D. B. Campbell; Rolf B. Dyce


The Astronomical Journal | 1971

General Relativity and the Orbit of Icarus

I. I. Shapiro; William B. Smith; Michael E. Ash; Samuel Herrick


Physical Review Letters | 1968

ICARUS: FURTHER CONFIRMATION OF THE RELATIVISTIC PERIHELION PRECESSION.

I. I. Shapiro; Michael E. Ash; William B. Smith

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Gordon H. Pettengill

Massachusetts Institute of Technology

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Richard P. Ingalls

Massachusetts Institute of Technology

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Irwin I. Shapiro

Massachusetts Institute of Technology

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William B. Smith

Massachusetts Institute of Technology

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Alan E. E. Rogers

Massachusetts Institute of Technology

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Charles C. Counselman

Massachusetts Institute of Technology

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L.P. Rainville

Massachusetts Institute of Technology

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M. A. Slade

Massachusetts Institute of Technology

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