A discussion of Halphen's method for secular perturbations and its application to the determination of long range effects in the motions of celestial bodies. Part 1

LDR 01163cam a2200289Ka 4500
001 011432969
003 MiAaHDL
005 20141013010000.0
006 m d
007 cr bn ---auaua
008 970103s1963 dcua b 000 0 eng d
035 ⊔ ⊔ ‡asdr-uiuc6389743
035 ⊔ ⊔ ‡a(OCoLC)36157773
040 ⊔ ⊔ ‡aGZM ‡cGZM ‡dBUF ‡dEGM ‡dOCLCQ ‡dOCLCG
043 ⊔ ⊔ ‡azmo----
049 ⊔ ⊔ ‡aUIUU
050 ⊔ 4 ‡aTL521 ‡b.A3312 no. 176
086 0 ⊔ ‡aNAS 1.12:176
100 1 ⊔ ‡aMusen, Peter, ‡d1912-
245 1 2 ‡aA discussion of Halphen's method for secular perturbations and its application to the determination of long range effects in the motions of celestial bodies. ‡nPart 1 / ‡cby Peter Musen.
260 ⊔ ⊔ ‡aWashington, D.C. : ‡bNational Aeronautics and Space Administration, ‡c1963.
300 ⊔ ⊔ ‡aiii, 52 p. : ‡bill. ; ‡c27 cm.
490 0 ⊔ ‡aNASA technical report ; ‡vNASA TR R-176
504 ⊔ ⊔ ‡aIncludes bibliographical references (p. 47).
538 ⊔ ⊔ ‡aMode of access: Internet.
650 ⊔ 0 ‡aGaussian quadrature formulas.
650 ⊔ 0 ‡aArtificial satellites ‡xOrbits.
651 ⊔ 0 ‡aMoon ‡xOrbit.
710 2 ⊔ ‡aGoddard Space Flight Center.
710 1 ⊔ ‡aUnited States. ‡bNational Aeronautics and Space Administration.
CID ⊔ ⊔ ‡a011432969
DAT 0 ⊔ ‡a20101101110006.0 ‡b20141013010000.0
DAT 1 ⊔ ‡a20141112173021.0 ‡b2023-03-14T18:25:04Z
CAT ⊔ ⊔ ‡aSDR-UIUC ‡dUNKNOWN ‡lloader.pl-003-020
FMT ⊔ ⊔ ‡aBK
HOL ⊔ ⊔ ‡0sdr-uiuc6389743 ‡auiug ‡bSDR ‡cUIUC ‡puiug.30112106682021 ‡sUIU ‡16389743
974 ⊔ ⊔ ‡bUIU ‡cUIUC ‡d20230314 ‡sgoogle ‡uuiug.30112106682021 ‡y1963 ‡rpd ‡qren