Eugene Rabe
German astronomer
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Physics
Eugene Rabe's Degrees
- PhD Astrophysics University of Göttingen
Why Is Eugene Rabe Influential?
(Suggest an Edit or Addition)According to Wikipedia, Eugene Karl Rabe was a German-American astronomer. He was born in Berlin, Germany, the son of Hermann and Luise. From 1937–1948 he was a member of the staff at the Heidelberg, Germany branch of the Astronomisches Rechen-Institut. After World War II it was arranged for him to come to the United States. He then became professor of astronomy at the University of Cincinnati, while working at the Cincinnati Observatory. His work included orbital motions of the Trojan asteroids, and particularly the orbit of 433 Eros. In 1951, he used twenty years worth of observations of Eros to determine the gravitational perturbations of the planets. From these, he calculated the most accurate masses to that date of Mercury, Venus, Mars and the Moon.
Eugene Rabe's Published Works
Published Works
- DETERMINATION AND SURVEY OF PERIODIC TROJAN ORBITS IN THE RESTRICTED PROBLEM OF THREE BODIES (1961) (122)
- Derivation of fundamental astronomical constants from the observations of Eros during 1926-1945 (1950) (51)
- Third-order stability of the long-period Trojan librations. (1967) (28)
- The Trojans as escaped satellites of Jupiter (1954) (18)
- ADDITIONAL PERIODIC TROJAN ORBITS AND FURTHER STUDIES OF THEIR STABILITY FEATURES (1962) (18)
- PERIODIC TROJAN ORBITS FOR THE RESONANCE 1/12, (1969) (15)
- Orbital Characteristics of Comets Passing through the 1:1 Commensurability with Jupiter (1972) (14)
- Elliptic Restricted Problem: Fourth-Order Stability Analysis of the Triangular Points (1973) (11)
- Plasmasphere response to the onset of quiet magnetic conditions: Plasma convection patterns (1977) (11)
- The earth+moon mass and other astronomical constants from the Eros motion 1926-1965 (1967) (11)
- Two New Classes of Periodic Trojan Librations in the Elliptic Restricted Problem and Their Stabilities (1970) (10)
- Further Studies on the Orbital Development of Pluto. (1957) (8)
- On the Origin of Pluto and the Masses of the Protoplanets. (1957) (7)
- Limiting Eccentricities for Stable Trojan Librations. (1965) (6)
- The precessional constant from Eros. (1950) (6)
- Corrected derivation of astronomical constants from the observations of Eros 1926-1945 (1967) (6)
- Additional note on the solar parallax from Eros (1954) (6)
- Motion of Eros and the astronomical unit (1967) (5)
- Trojans and Comets of the Jupiter Group (1971) (5)
- Stability Characteristics of the Short-Period Trojan Librations (1968) (4)
- The orbital motion of the minor planet (1362) Griqua and the mass of Jupiter. (1959) (3)
- Existence of four families of commensurability- related periodic Trojan orbits. (1967) (2)
- Perihelion Longitudes and Jacobi Constants of Jupiter Group Comets as Indicators of Their Possible Origin from the Two Equilateral Trojan Clouds (1974) (2)
- The orbit of (1011) Laodamia and the mass of Mars. (1959) (2)
- On the compatibility of the recent solar parallax results from radar echoes of Venus with the motion of Eros (1965) (1)
- Escaping satellites of Jupiter. (1954) (1)
- On the Formation of Rapidly Rotating. Asteroids. (1960) (1)
- Proceedings of the Celestial Mechanics Conference: Secular perturbations of the protoplanets (1958) (1)
- A method for stability determinations in the elliptic restricted problem (1970) (0)
- Some Remarks on the Further Improvement, by Conventional and New Methods, of Astronomical Constants involved in Ephemeris Computation (1962) (0)
- The Use of Asteroids for Determinations of Masses and Other Fundamental Constants (1971) (0)
- 1452 = 1938 DZ1 : Improved Ephemeris for 1950 (1949) (0)
- Parameter distribution of small periodic librations about the equilateral points of the elliptic restricted problem (1973) (0)
- Periodic Trojan orbits in the elliptic restricted problem. (1966) (0)
- A New Class of Long-Period Trojan Librations. (1965) (0)
- Some remarks on the paper by B. G. Marsden “An attempt to reconcile the dynamical and radar determinations of the Astronomical Unit” (1965) (0)
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