Scholarly record
THE SOFTWARE COMPLEX FOR COMPUTER SIMULATING THE OBSERVATION OF STARS FROM THE LUNAR SURFACE AND CALCULATING THEIR SELENOGRAPHICAL COORDINATES
Abstract
Appointment of the software system is the solving the direct and inverse problem of the lunar physical libration. The direct problem is to calculate the selenographic coordinates of stars falling within the field of view of the telescope mounted on one of the lunar poles. The analytic theory of the physical libration of the Moon of Petrova N. [1] provides the base for the solution of the problem. The inverse problem is to determine the parameters of lunar physical libration based on the simulated "observable" selenographic coordinates of stars. In the development of software system, the modern methods of structural and object-oriented programming are applied using properties and methods of Excel - workbooks, sheets, cells and charts. The software package includes several Excel workbooks, interconnected by means of program modules written in the VBA. The Excel books form a kind of database, which provides the solving of both problems by necessary information. The software package allows analyzing the trajectories of stars in future observations, as well as testing the sensitivity of the selenographic coordinates to the parameters of the internal structure of the Moon.
Publication Impact Profile
Publication details
References14
Petrova N. Analytical extension of Lunar libration tables. Earth, Moon and Planets, Vol. 73, No 1, pp. 71-99, 1996.
Hanada H. Application of a PZT telescope to In situ Lunar Orientation Measurement (ILOM) Proc. of Int. Assoc. Geodesy. IAG GA, Sapporo, Japan, June 30 – July 11. – 2003. – Springer. – pp. 163 – 168.
Moons, M. Analytical theory of libration of the Moon, Celest. Mech. & Dyn. Astr., 26, 131, 1982.
Eckhardt D.H. Theory of the libration of the Moon. // The Moon & the Planets, 1981, 25, pp. 3 – 50.
Chapront J., Chapront –Touzé M. Lunar motion: theory and observations. Cel. Mech. & Dyn. Astron., v.66, pp 31-38, 1997.
Chapront J., Chapront –Touzé M., Francou G. Complements to Moon’s Lunar libration theory. Cel. Mech. & Dyn. Astron., v.73, pp 317-328, 1999.
Rambaux N., J. G. Williams The Moon’s physical librations and determination of their free modes. // Celest Mech Dyn Astr, 2011. 109:85–100.
Petrova N., Hanada H. Computer simulation of observations of stars from the Moon using the polar zenith telescope of the Japanese project ILOM, Solar System Research, 2012, Vol. 47, No. 6, pp. 463–476.
Petrova, N., Abdulmyanov T., Hanada H. Some qualitative manifestations of the physical libration of the Moon by observing stars from the lunar surface. //J. Adv. Space Res., 2012. V. 50, pp. 1702 1711
Demidovich, B. and Maron, I., Osnovy vychislitel’noi matematiki (Foundations of Calculus Mathematics), St. Petersburg: Lan’, 2006.
Dickey, J.O., Bender, P.L., Newhall, X.X., et al., Lunar laser ranging: a continuing legacy of the apollo program, Science, 1994, vol. 265, p. 482.
Lemoine F.G., D.S.Smith, M.T.Zuber, G.A. Neumann, D.D.Rowlands. A 70th degree lunar gravity model (GLGM-2) from Clementine and other tracking data. // JGR, 1997. v.102, № E7, p.16, 339-16,359.
Konopliv, A. S., LP L RSS line of sight acceleration profiles V1.0, LP-L-RSS-5-LOS-V1.0, //NASA Planetary Data System, 2000 (LP150Q –model).
Matsumoto K., Goossens S., Ishihara Y., et al. An improved lunar gravity field model from SELENE and historical tracking data: Revealing the farside gravity features. //JGR, 2010. 115, E06007, 20 pp.
View or Download full articleAccess options
SWS access login
Login as SWS Scientific CommitteeLogin as SWS Scientific PartnerLogin as SWS AuthorAuthors and approved SWS contributors will read and export their own linked papers after identity matching by SWS profile, email and SGEM GlobalID.
For librarian assistance: [email protected]
Purchase Instant Access
- Article can be downloaded after successful payment.
- Article may be used according to SWS library access terms.
- Article cannot be redistributed.


