Search arXivSearch

arXiv · 2502.07831

Endurance Science Workshop 2023 Final Report

Abstract

Endurance is a mission concept to explore and ultimately return samples from the Moon's largest and oldest impact basin, South Pole-Aitken (SPA). SPA holds the answers to many outstanding planetary science questions, including the earliest impact bombardment of the Solar System and the evolution of the Moon's interior. Endurance would address these questions by traversing 2,000 kilometers across the lunar farside, collecting samples, and delivering those samples to Artemis astronauts for return to Earth. Endurance was identified as the highest priority strategic mission for NASA's Lunar Discovery and Program in the recent Planetary Science and Astrobiology Decadal Survey. This report summarizes the results from the first public workshop about the concept. Major findings include: (1) Endurance is an exciting concept that would address long-standing, high-priority lunar and planetary science questions, and the community is ready for it. (2) Endurance's sample science objectives are achievable, although they would require coordinated analysis techniques and numerous diverse samples. (3) Geologic context is essential for addressing Endurance's science objectives. (4) While Endurance's objectives center on sample return, Endurance's long traverse would enable a variety of additional transformative science investigations. (5) Endurance is an ambitious mission that would be enabled and enhanced by investing in developing key technologies now. (6) Endurance should strive to include more diverse perspectives in its formulation, particularly from early-career scientists and engineers who will ultimately operate the rover and analyze the samples. Endurance is early in its formulation and the next major activity will be a Science Definition Team (SDT). It is expected that this report and the findings therein may be useful input to the Endurance SDT.

Explore related subjects

Keep this discovery

Explore connections, maps & timelines

BibTeXRIS

James Tuttle Keane, Barbara Cohen, Carolyn Crow, Benjamin Greenhagen, Bradley Jolliff, Yang Liu, Charles Shearer, Sonia Tikoo, Sarah Valencia. 2025-02-11. Endurance Science Workshop 2023 Final Report. https://arxiv.org/abs/2502.07831

Cite the original work for its findings. Save a collection to share your selection of sources.

KEEP EXPLORING

Related papers

Performance characterization of a new Structural and Thermal Architecture for a future spaceborne Closed-Cycle Dilution Refrigerator

A Structural and Thermal Model (STM) has been developed to support the new spaceborne Closed-Cycle Dilution Refrigerator (CCDR), which aims to provide continuous cooling at 100~mK for long-duration astrophysical missions. The STM is based on a hexapod architecture that ensures both thermal decoupling and mechanical robustness during launch. In this paper, we present the characterization of its thermal and mechanical performances. A dedicated experimental setup was used to investigate the thermal behavior of the STM across a broad temperature range. The study reveals limitations of the collar design, with incomplete power interception from thermal boundary resistances and vibration test failure traced to defective strut gluing. These results guide the next STM iteration with optimized collar and strut assembly for reliable CCDR operation in space.

astro-ph.IM

The Simons Observatory: Development of a Pipeline to Detect Rapid Transients in Time-Ordered Data

We introduce a method for detecting astrophysical transients evolving on timescales of milliseconds to minutes using cosmic microwave background (CMB) survey telescopes. While previous transient searches in CMB data operate in map space, our pipeline directly processes the raw time-ordered data, enabling sensitivity to fast, dynamic signals. We integrate our detection approach into the Simons Observatory time-domain pipeline and assess the performance by injecting symmetric, stellar flare-like light curves into simulated observations. For events flaring with a timescale of 0.5 s, the pipeline detects $\gtrsim90$ % of events at flux densities of 800, 1150, 1650, and 4250\,mJy when measured in the 93, 145, 225, and 280 GHz bands respectively. At a fixed peak flux density, the pipeline more readily detects longer flares. The limiting flux density for 90 % completeness is four times lower for a $\ge5$ s flare than for a 0.5 s flare, while the flux density limits for $\gtrsim50$ % detection efficiency are comparable to the rms noise of the time-ordered data. We are able to determine the position of detected events in each observing band, with a positional uncertainty at the detection threshold comparable to the telescope resolution at that band. These results demonstrate the readiness of this pipeline for incorporation into upcoming Simons Observatory data analyses.

astro-ph.IM

Thermal conductivity of various CFRPs from 100 mK to 20 K

Carbon-fiber-reinforced polymers (CFRPs) are some of the most useful materials for building spacecraft and aerospace tools. They are especially valuable for systems that work at extremely cold (cryogenic) temperatures because they are strong, lightweight, and don't transfer heat easily. In this study, researchers measured how well heat moves through several different types of carbon fiber samples, specifically T300, T700, HS40, M55J, and IMA, at different fiber layouts and densities. These measurements were taken at ultra-cold temperatures ranging from 100 mK to 20 K. The team used a newly developed analysis method to calculate the thermal conductivity for each sample. Finally, they shared how each material behaved at different temperatures and compared their findings to previous research.

astro-ph.IM