Semi-Analytical Lunar Ephemeris — The Main Problem

1979 ◽  
pp. 73-75 ◽  
Author(s):  
Jacques Henrard
Keyword(s):  
1971 ◽  
Author(s):  
Andre Deprit ◽  
Jacques Henrard ◽  
Arnold Rom
Keyword(s):  

1962 ◽  
Vol 11 (2) ◽  
pp. 90-90

Parmi les résolutions et recommandations adoptées par les Commissions et Sous-Commissions, seules sont reproduites ici celles qui présentent un vaste intérêt et s’adressent à une large audience; les autres peuvent être trouvées dans les Comptes-Rendus de réunions, auxquels nous renvoyons. Là où ils sont donnés, les numéros des résolutions sont ceux utilisés dans les Comptes- Rendus.Commission 4—voir page 167. (Voir aussi Commission 31.)2. La valeur provisoire du temps des éphémérides, obtenue en comparant la longitude moyenne de la Lune résultant d’observations rapportées à l’équinoxe du FK 4, avec les positions données par 1’Improved Lunar Ephemeris est appelée T.E.O. La différence T.E.O. — T.u.2 est appelée Δ T0.


1972 ◽  
Vol 47 ◽  
pp. 395-401
Author(s):  
L. V. Morrison

Analyses of occultation timings show that periodic correction terms with semi-amplitude as great as 0.″18 arise from corrections required to the empirical constants of the Brown/Eckert theory. Using the atomic time-scale, some of the occultation data have been used to determine a correction of – 30 ± 16″/cy2 to Spencer Jones' value for the secular acceleration of the Moon. In the light of this correction, and previous determinations, attention is drawn to the possible weakness of Spencer Jones' value, which is not reflected in his quoted error of ± 1″/cy2. Further analyses of 50000 occultations observed since 1943 promise to reveal more accurately-determined corrections.


1971 ◽  
Vol 76 ◽  
pp. 273 ◽  
Author(s):  
Andre Deprit ◽  
Jacques Henrard ◽  
Arnold Rom
Keyword(s):  

1970 ◽  
Vol 75 ◽  
pp. 747 ◽  
Author(s):  
Andre Deprit ◽  
Jacques Henrard ◽  
Arnold Rom
Keyword(s):  

1973 ◽  
Vol 2 (4) ◽  
pp. 203-206
Author(s):  
J. McK. Luck ◽  
M. J. Miller ◽  
P. J. Morgan

The Division of National Mapping has received, on long term loan from NASA and in co-operation with the Smithsonian Astrophysical Observatory, a Lunar Laser Ranging instrument consisting of a gigawatt pulsed ruby laser, a 150 cm aspheric Ritchey-Chretien telescope, and associated electronic equipment. The instrument was formerly operated by the Air Force Cambridge Research Laboratories at Mount Lemmon in Arizona. Its principal use by National Mapping will be direct determination of the distance between the telescope and any of the three retro-reflector arrays placed on the Moon at Hadley’s Rille, Fra Mauro and Mare Tranquillitatis by Apollo astronauts. Full scale operation in conjunction with similar instruments well separated in latitude and longitude, in particular at Mount McDonald in Texas and Mount Haleakala in Hawaii, will permit determination of Earth rotation and polar motion, lunar ephemeris and libration, and tectonic plate movement or continental drift, which justifies its use in a geodetic environment.


Science ◽  
1970 ◽  
Vol 168 (3939) ◽  
pp. 1569-1570 ◽  
Author(s):  
A. Deprit ◽  
J. Henrard ◽  
A. Rom
Keyword(s):  

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