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Laser Ranging to the Lost Lunokhod~1 Reflector

Published 28 Sep 2010 in astro-ph.EP | (1009.5720v2)

Abstract: In 1970, the Soviet Lunokhod 1 rover delivered a French-built laser reflector to the Moon. Although a few range measurements were made within three months of its landing, these measurements---and any that may have followed---are unpublished and unavailable. The Lunokhod 1 reflector was, therefore, effectively lost until March of 2010 when images from the Lunar Reconnaissance Orbiter (LRO) provided a positive identification of the rover and determined its coordinates with uncertainties of about 100 m. This allowed the Apache Point Observatory Lunar Laser-ranging Operation (APOLLO) to quickly acquire a laser signal. The reflector appears to be in excellent condition, delivering a signal roughly four times stronger than its twin reflector on the Lunokhod 2 rover. The Lunokhod 1 reflector is especially valuable for science because it is closer to the Moon's limb than any of the other reflectors and, unlike the Lunokhod 2 reflector, we find that it is usable during the lunar day. We report the selenographic position of the reflector to few-centimeter accuracy, comment on the health of the reflector, and illustrate the value of this reflector for achieving science goals.

Citations (66)

Summary

Laser Ranging to the Lost Lunokhod 1 Reflector: An Evaluation

The research paper titled "Laser Ranging to the Lost Lunokhod 1 Reflector" by Murphy et al. explores the rediscovery and subsequent measurements of the Lunokhod 1 laser reflector, initially delivered to the Moon by the Soviet Lunokhod 1 rover in 1970. For nearly four decades, effective ranging to this reflector was not possible, primarily due to uncertainties surrounding its exact location. This paper details how images from the Lunar Reconnaissance Orbiter (LRO) in 2010 facilitated a significant breakthrough in relocating this lunar asset.

The successful identification and the precise coordinates of the Lunokhod 1 reflector emerged from analysis of LRO Camera images and Lunar Orbiter Laser Altimeter data. Once rediscovered, the Apache Point Observatory Lunar Laser-ranging Operation (APOLLO) commenced laser ranging operations, revealing that the Lunokhod 1 reflector was in excellent condition, yielding a signal notably stronger than its counterpart, Lunokhod 2. This finding is significant due to Lunokhod 1's close proximity to the Moon's limb, enabling enhanced sensitivity to selenographic positioning.

Observations and Measurements

The research emphasizes observational data collected between April and August 2010, detailing several ranging sessions to ascertain the position of the Lunokhod 1 reflector with centimeter-level accuracy. Reflectors from the Apollo missions, alongside Lunokhod 1 and 2, were used to fine-tune lunar orientation measurements, allowing better calculation of Moon's internal structure and gravitational dynamics.

Table~\ref{tab:obs} within the paper collates key observation metrics, including solar elevation and libration at each measurement instance. Initial returns from Lunokhod 1 were unexpectedly strong, suggesting operational health superior to its counterpart Lunokhod 2, which showcased greater degradation over time.

Positional Analysis

The study employs a range of technical adjustments, such as accounting for lunar tidal deformation and recalibrating lunar orientation, to ensure the accuracy of the Lunokhod 1 position. Precision was further refined through least-squares method fitting, cumulating in ascertaining coordinates in both spherical and Cartesian systems relative to the Jet Propulsion Laboratory's DE421 ephemeris.

The Lunokhod 1 reflector's coordinates, derived with extreme precision, are listed alongside other lunar reflectors, highlighting their static offsets and relevance within lunar orientation frameworks.

Reflector Performance

A comparative assessment reveals the Lunokhod 1 reflector outperforming expectations concerning return rates, particularly when compared to Lunokhod 2. In conditions void of sunlight, Lunokhod 1 exhibited approximately fourfold higher return levels than Lunokhod 2. This disparity prompts further investigation into the degradation mechanisms affecting lunar reflectors, with current theories suggesting differences in the exposure and environmental interactions over the lunar surface as causal factors.

Scientific and Future Implications

The meticulous recovery and ranging of the Lunokhod 1 reflector bear significant implications for lunar laser ranging (LLR) experiments. This newly acquired data enhances precision in lunar orientation, gravitational testing, and potential tidal deformation modeling. Lunokhod 1's advantageous position relative to the Earth's line of sight augments existing lunar science capabilities, reaffirming its role as a pivotal reflector amidst the broader lunar network.

In conclusion, the successful ranging to Lunokhod 1 rejuvenates legacy scientific instruments, expanding the frontier of lunar exploration and gravitational studies. Continued monitoring and data collation promise deeper understanding of both lunar and broader celestial mechanics, paving the way for advances in both theoretical models and practical applications within astrophysics and planetary science. Future efforts are likely to focus on integrating these findings into comprehensive models of lunar dynamics, potentially inspiring new methodologies in precision laser ranging technology.

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