Elena V. Pitjeva
Elena Vladimirovna Pitjeva (Елена Владимировна Питьева) is a Russian astronomer working at the
She began employment activity as an engineer-observer at the Astrophysical observation station of the Astronomical Observatory of
Major research interests of Pitjeva include the construction of numerical ephemerides of the planets, the determination of the planets' and asteroids' masses, the parameters of planet rotation and planetary topography, the solar corona and oblateness and general relativity testing. She is one of creators of the numerical Ephemerides of Planets and the Moon (EPM) of IAA RAS that originated in the seventies of the past century and have been developed since that time. The version of the EPM2004 ephemeris has been adopted as the ephemeris basis of Russian Astronomical Yearbook since 2006. The updated EPM2008 ephemerides are available to outside users via ftp.[2]
The works of Pitjeva have recently been used by several scientists to test several models of modified gravity in the Solar System. Pitjeva has also contributed to a better understanding an influence of asteroids and
Education
Pitjeva graduated from the Faculty of Mathematical and Mechanical at
Publications (selection)
- Pitjeva, E. V. (2010). "Influence of trans-neptunian objects on motion of major planets and limitation on the total TNO mass from planet and spacecraft". Proc. IAU Symp. No. 263/ Icy bodies of the solar system //D. Lazzaro, D. Prialnik, R. Schulz, J. A. Fernandez (eds.), Cambridge University Press. pp. 93–97.
- Pitjeva, E. V. (2010). "EPM ephemerides and relativity". Proc. IAU Symp. No. 261 / Relativity in fundamental astronomy: dynamics, reference frame, and data analysis //S. Klioner, P.K. Seidelmann, M. Soffel (eds.), Cambridge University Press. pp. 170–178.
- Pitjeva, E. V.; S2CID 121374703.
- Pitjeva, E. V. (2009). "Ephemerides EPM2008: the updated model, constants, data" (PDF). Proceedings of the "Journees 2008 Systemes de reference spatio-temporels", M. Soffel and N. Capitaine (eds.), Lohrmann-Observatorium and Observatoire de Paris. pp. 57–60. Archived from the original (PDF) on 2011-06-07.
- Khriplovich, I. B.; Pitjeva, E. V. (2006). "Upper limits on density of dark matter in Solar System". S2CID 8996172.
- Pitjeva, E. V. (2005). "High-Precision Ephemerides of Planets—EPM and Determination of Some Astronomical Constants" (PDF). Solar System Research. 39 (3): 176–186. S2CID 120467483. Archived from the original(PDF) on 2008-10-31.
- Pitjeva, E. V. (2005). "Relativistic Effects and Solar Oblateness from Radar Observations of Planets and Spacecraft". Astronomy Letters. 31 (5): 340–349. S2CID 54645688.
- Pitjeva, E. V. (2004). "Estimations of masses of the largest asteroids and the main asteroid belt from ranging to planets, Mars orbiters and landers". 35th COSPAR Scientific Assembly. Held 18–25 July 2004, in Bibcode:2004cosp...35.2014P.
- .
- Pitjeva, E. V. (2001). "Modern numerical ephemerides of planets and the importance of ranging observations for their creation". S2CID 118759118.
Bibliometric information
According to the
References
- ^ Institute Applied Astronomy RAS (2006-08-23). "Laboratory of Ephemeris Astronomy". Archived from the original on 2011-06-22. Retrieved 2010-05-12.
- ^ Institute Applied Astronomy RAS (2006-08-23). "EPM2008". Retrieved 2010-05-12.[permanent dead link]
- ^ IAU WG NSFA. "Current Best Estimates". Archived from the original on 2009-12-08. Retrieved 2010-05-12.
- ^ International Astronomical Union. "IAU Commission 4 Membership". Archived from the original on 2010-04-12. Retrieved 2010-05-12.
- ^ International Astronomical Union. "IAU Commission 52 Membership". Retrieved 2010-05-12.
- ^ International Astronomical Union. "WG IAU NSFA Membership". Retrieved 2010-05-12.
External links
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