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VIPER Mission Traverse Planning – Design, Strategies, and DynamicsThe Volatiles Investigation Polar Exploration Rover (VIPER) is a lunar polar volatiles prospecting mission developed through NASA’s Science Mission Directorate (SMD) Planetary Science Di-vision[1].VIPER is scheduled to land on Mons Mouton near the lunar South Pole in late 2024. VIPER’s primary mission goal is to characterize the distribution of water and volatiles across a range of thermal environments. This characterization aims to assist in understanding the origin of lunar polar volatiles and also help evaluate the In-Situ Resource Utilization (ISRU) potential of the lunar poles.

The VIPER rover is a four-wheeled robotic vehicle weighing ~450 kg. It is solar-powered and teleoperated from Earth over a line-of-sight radio link. The rover can move at up to 20 cm/s on flat terrain. Accounting for commanding, localization, navigation, and obstacle-avoidance delays, however, the effective speed is closer to 1 cm/s. This effective speed is known as “Speed Made Good” (SMG), adopted from maritime culture, and kept as a key performance metric for VIPER oper-ations planning, execution, and evaluation.

The mission duration is anticipated to be more than 90 Earth days and involves up to 20 km of driving. VIPER’s prospecting payload consists of spectrometers to detect volatiles and assess concentrations, context imagers, and a drill for sub-surface measurements down to one meter depth [2]. Mobility, combined with the prospecting and drill instrument suite, makes VIPER an analytically powerful resource mapper.
Document ID
20230004239
Acquisition Source
Ames Research Center
Document Type
Extended Abstract
Authors
K Ennico Smith
(Ames Research Center Mountain View, California, United States)
A Colaprete
(Ames Research Center Mountain View, California, United States)
M Shirley
(Ames Research Center Mountain View, California, United States)
E Balaban
(Ames Research Center Mountain View, California, United States)
R Beyer
(SETI Institute Mountain View, California, United States)
K Bradner
(Ames Research Center Mountain View, California, United States)
J Coyan
(United States Geological Survey Reston, Virginia, United States)
R C Elphic
(Ames Research Center Mountain View, California, United States)
L Falcone
(Wyle (United States) El Segundo, California, United States)
C Fassett
(APL)
D Lees
(Ames Research Center Mountain View, California, United States)
D S S Lim
(Ames Research Center Mountain View, California, United States)
Z Mirmalek
(Bay Area Environmental Research Institute Petaluma, California, United States)
A. Nefian
(Ames Research Center Mountain View, California, United States)
M Siegler ORCID
(Planetary Science Institute Tucson, Arizona, United States)
Date Acquired
March 30, 2023
Subject Category
Astrophysics
Meeting Information
Meeting: 23rd Meeting of the Space Resources Roundtable (SRR)
Location: Golden, CO
Country: US
Start Date: June 6, 2023
End Date: June 9, 2023
Sponsors: Colorado School of Mines
Funding Number(s)
WBS: 993436.04.01
Distribution Limits
Public
Copyright
Portions of document may include copyright protected material.
Technical Review
Single Expert
Keywords
Volatiles Investigation Polar Exploration Rover (VIPER)
Mons Mouton
lunar South Pole
Thermal Environments
origin of lunar polar volatiles
In-Situ Resource Utilization (ISRU)
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