Orbit Design for the Millimetron Space Observatory
T. A. Syachina, A. G. Rudnitskiy, P. V. Mzhelskiy, M. A. Shchurov, P., R. Zapevalin

TL;DR
This paper details the orbit design process for the Millimetron space observatory, integrating technical and scientific constraints, and demonstrating its scientific capabilities through VLBI simulations.
Contribution
It introduces a numerical integration approach for orbit design, improving accuracy over previous analytical methods, and provides detailed mission trajectory planning.
Findings
Successful orbit selection and transfer planning.
Feasibility of scientific objectives confirmed through VLBI simulations.
Precise timing for mission milestones established.
Abstract
Millimetron is a space observatory for millimeter and sub-millimeter observations planned for launch around 2030. The 10-meter diameter space unfolded telescope will be cooled down to 10~K and operated in the vicinity of Lagrange point L2. Mission lifetime is 10 years and it includes astronomical observations in two modes: as a space-ground interferometer and as a single-dish telescope. This paper presents the results of the Millimetron space observatory orbit design that takes into account technical and scientific requirements and constraints. It covers the computation of suitable operational orbits, the selection of an orbit, and the transfer from Earth. Furthermore, scientific objectives are demonstrated through VLBI visibility simulation and image reconstruction. Unlike previous works that used analytical methods, this work employs numerical integration for orbital design. Based on…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsAstronomy and Astrophysical Research · History and Developments in Astronomy · Space Satellite Systems and Control
