3.5-meter Segmented-Mirror Robotic Space Telescope Mission White Paper IV. Key Scientific Mission: Solar-System Small Bodies and Planetary Defense
Abstract
The baseline 0.2--1.5 μm observatory provides rapid-response astrometry, visible and near-infrared taxonomy, rotation and phase curves, recovery, and long-arc orbit improvement for near-Earth objects and other small bodies. The instrument study also evaluates calibrated throughput to 2.70 μm with a 3.0 μm operational band-edge goal. A reduction to 2.5 μm remains the formal engineering off-ramp if thermal, detector, cooling, mass, power, or cost constraints require it. The 3.5-meter Segmented-Mirror Robotic Space Telescope does not carry a mid-infrared channel. Coordinated ground-based mid-infrared telescopes provide the thermal fluxes required to infer diameter and albedo, while the space mission supplies contemporaneous reflected-light measurements and observing geometry. The program combines recovery, physical characterization, orbit refinement, and covariance-based hazard assessment. Its CODES dynamics system and OGFinder-to-OpenOrb processing path connect measured astrometry to reproducible orbit solutions and close-approach predictions.
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BibTeX
@misc{kim202635meter,
title = {{3.5-meter Segmented-Mirror Robotic Space Telescope Mission White Paper IV. Key Scientific Mission: Solar-System Small Bodies and Planetary Defense}},
author = {Juhan Kim and Yong-Woo Kang and Sang Hyun Lee and Jeong-Yeol Han and Sungwook E. Hong and Bongkon Moon and Donguk Song and Juhyung Kang and Myeong-Gu Park and Sang Chul Kim and Chung-Uk Lee and Sangmo Tony Sohn and Arman Shafieloo and David Parkinson and Hong Soo Park and Dohyeong Kim and Chan Park and Jungjoo Sohn and Young-Beom Jeon and Jong-Hak Woo and Hyung Mok Lee and Hong Bae Ann and Myungkook James Jee and Mansoo Choi and Changbom Park},
howpublished = {arXiv},
year = {2026},
month = sep,
doi = {10.48550/arxiv.2609.03371},
eprint = {2609.03371},
archivePrefix = {arXiv},
url = {https://arxiv.org/abs/2609.03371},
}
RIS
TY - UNPB
TI - 3.5-meter Segmented-Mirror Robotic Space Telescope Mission White Paper IV. Key Scientific Mission: Solar-System Small Bodies and Planetary Defense
AU - Juhan Kim
AU - Yong-Woo Kang
AU - Sang Hyun Lee
AU - Jeong-Yeol Han
AU - Sungwook E. Hong
AU - Bongkon Moon
AU - Donguk Song
AU - Juhyung Kang
AU - Myeong-Gu Park
AU - Sang Chul Kim
AU - Chung-Uk Lee
AU - Sangmo Tony Sohn
AU - Arman Shafieloo
AU - David Parkinson
AU - Hong Soo Park
AU - Dohyeong Kim
AU - Chan Park
AU - Jungjoo Sohn
AU - Young-Beom Jeon
AU - Jong-Hak Woo
AU - Hyung Mok Lee
AU - Hong Bae Ann
AU - Myungkook James Jee
AU - Mansoo Choi
AU - Changbom Park
PY - 2026
DA - 2026/09/17
PB - arXiv
DO - 10.48550/arxiv.2609.03371
UR - https://arxiv.org/abs/2609.03371
AB - The baseline 0.2--1.5 μm observatory provides rapid-response astrometry, visible and near-infrared taxonomy, rotation and phase curves, recovery, and long-arc orbit improvement for near-Earth objects and other small bodies. The instrument study also evaluates calibrated throughput to 2.70 μm with a 3.0 μm operational band-edge goal. A reduction to 2.5 μm remains the formal engineering off-ramp if thermal, detector, cooling, mass, power, or cost constraints require it. The 3.5-meter Segmented-Mirror Robotic Space Telescope does not carry a mid-infrared channel. Coordinated ground-based mid-infrared telescopes provide the thermal fluxes required to infer diameter and albedo, while the space mission supplies contemporaneous reflected-light measurements and observing geometry. The program combines recovery, physical characterization, orbit refinement, and covariance-based hazard assessment. Its CODES dynamics system and OGFinder-to-OpenOrb processing path connect measured astrometry to reproducible orbit solutions and close-approach predictions.
ER -