火星周回衛星、20年を経て新たな機動を獲得(NASA Mars Orbiter Learns New Moves After Nearly 20 Years in Space)

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2025-06-26 NASA

NASAの火星探査機MROは、約20年の運用を経て新たな操縦「非常に大きなロール(最大120度)」を導入し、地下レーダーSHARADの性能を強化。これにより、探査機の構造による干渉を避け、より深く鮮明な地下構造や氷層(最大2km)を観測可能にした。従来比で約10倍の信号強度を達成。設計寿命を超えて活躍するMROに新たな科学的価値を付加する成果であり、年1〜2回の実施が計画されている。

<関連情報>

SHARADはMRO宇宙船の超大型ロールからの加速により火星のより深い地下構造を照らし出す SHARAD Illuminates Deeper Martian Subsurface Structures with a Boost from Very Large Rolls of the MRO Spacecraft

Nathaniel E. Putzig, Gareth A. Morgan, Matthew R. Perry, Bruce A. Campbell, Jennifer L. Whitten, Fabrizio Bernardini, Alessandro DiCarlofelice, Piero Tognolatti and Pierfrancesco Lombardo
The Planetary Science Journal  Published: 2025 June 11
DOI:10.3847/PSJ/addbe1

火星周回衛星、20年を経て新たな機動を獲得(NASA Mars Orbiter Learns New Moves After Nearly 20 Years in Space)

Abstract

Throughout its mission, the Mars Reconnaissance Orbiter (MRO) has often rolled about its along-track axis by up to 28° to partially compensate for the suboptimal location of the Shallow Radar (SHARAD) antenna along an edge of the spacecraft that is opposite the imaging payload deck, thereby enhancing the signal-to-noise ratio (S/N) of echoes returned from the surface. After recent modeling work predicted that a much larger roll would improve the S/N by ~10 dB relative to nadir-pointed observing, MRO began a limited series of 120° roll maneuvers to test the effects on radar sounding. Three such SHARAD very-large-roll (VLR) observations were acquired between 2023 May and 2024 September, and they show dramatic improvements in signal clarity and depth of penetration, with S/N increasing by 9, 11, and 14 dB over that of nearly coincident observations at 0° roll angle. In low dielectric terrains, the first and second VLR observations enabled basal detections at depths previously unachievable, reaching depths of 800 m in Medusae Fossae materials and 1500 m through the ice of Ultimi Scopuli, respectively. The second VLR observation also obtained enhanced reflections throughout the ice stack. In the higher dielectric terrain of Amazonis Planitia, the third VLR observation improved continuity of a dipping subsurface interface, but it revealed neither an extension of the interface to greater depths nor any deeper interfaces. The MRO mission intends to obtain more SHARAD VLR observations of polar terrains and of midlatitude glacial and ground ices, sediments, and volcanics.

1702地球物理及び地球化学
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