Report of the Joint Workshop on Induced Special Regions.


Journal

Life sciences in space research
ISSN: 2214-5532
Titre abrégé: Life Sci Space Res (Amst)
Pays: Netherlands
ID NLM: 101632373

Informations de publication

Date de publication:
Nov 2019
Historique:
received: 23 02 2019
revised: 18 09 2019
accepted: 19 09 2019
entrez: 4 12 2019
pubmed: 4 12 2019
medline: 11 5 2021
Statut: ppublish

Résumé

The Joint Workshop on Induced Special Regions convened scientists and planetary protection experts to assess the potential of inducing special regions through lander or rover activity. An Induced Special Region is defined as a place where the presence of the spacecraft could induce water activity and temperature to be sufficiently high and persist for long enough to plausibly harbor life. The questions the workshop participants addressed were: (1) What is a safe stand-off distance, or formula to derive a safe distance, to a purported special region? (2) Questions about RTGs (Radioisotope Thermoelectric Generator), other heat sources, and their ability to induce special regions. (3) Is it possible to have an infected area on Mars that does not contaminate the rest of Mars? The workshop participants reached a general consensus addressing the posed questions, in summary: (1) While a spacecraft on the surface of Mars may not be able to explore a special region during the prime mission, the safe stand-off distance would decrease with time because the sterilizing environment, that is the martian surface would progressively clean the exposed surfaces. However, the analysis supporting such an exploration should ensure that the risk to exposing interior portions of the spacecraft (i.e., essentially unsterilized) to the martian surface is minimized. (2) An RTG at the surface of Mars would not create a Special Region but the short-term result depends on kinetics of melting, freezing, deliquescence, and desiccation. While a buried RTG could induce a Special Region, it would not pose a long-term contamination threat to Mars, with the possible exception of a migrating RTG in an icy deposit. (3) Induced Special Regions can allow microbial replication to occur (by definition), but such replication at the surface is unlikely to globally contaminate Mars. An induced subsurface Special Region would be isolated and microbial transport away from subsurface site is highly improbable.

Identifiants

pubmed: 31791605
pii: S2214-5524(19)30116-6
doi: 10.1016/j.lssr.2019.09.002
pii:
doi:

Types de publication

Journal Article

Langues

eng

Sous-ensembles de citation

IM

Pagination

50-59

Informations de copyright

Copyright © 2019. Published by Elsevier Ltd.

Auteurs

Michael Meyer (M)

Science Mission Directorate, NASA HQ, Washington DC, United States. Electronic address: michael.a.meyer@nasa.gov.

Corien Bakermans (C)

Microbiology, Division of Mathematics and Natural Sciences, Penn State University, Altoona, United States.

David Beaty (D)

Mars Exploration Directorate, Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States.

Douglas Bernard (D)

Engineering and Science Directorate, Jet Propusion Laboratory, California Institute of Technology, Pasadena, United States.

Penelope Boston (P)

NASA Astrobiology Institute, Ames Research Center, Mountain View, United States.

Vincent Chevrier (V)

Arkansas Center for Space and Planetary Sciences, University of Arkansas, Fayetteville, United States.

Catharine Conley (C)

Science Mission Directorate, NASA HQ, Washington DC, United States.

Ingrid Feustel (I)

Chemical Control Division, US Environmental Protection Agency, Washington DC, United States.

Raina Gough (R)

Cooperative Institute for Research in Environmental Sciences, University of Colorado, Boulder, United States.

Timothy Glotch (T)

Department of Geosciences, Stony Brook University, Stony Brook, United States.

Lindsay Hays (L)

NASA Astrobiology Institute, Ames Research Center, Mountain View, United States.

Karen Junge (K)

Applied Physics Lab. University Washington, Seattle, United States.

Robert Lindberg (R)

Mechanical and Aerospace Engineering, University Virginia, Charlottesville, United States.

Michael Mellon (M)

Johns Hopkins Applied Physics Laboratory, Laurel, United States.

Michael Mischna (M)

Engineering and Science Directorate, Jet Propusion Laboratory, California Institute of Technology, Pasadena, United States.

Clive R Neal (CR)

College of Engineering, University Notre Dame, Notre Dame, United States.

Betsy Pugel (B)

Science Mission Directorate, NASA HQ, Washington DC, United States.

Richard Quinn (R)

Applied Physics Lab. University Washington, Seattle, United States.

Francois Raulin (F)

LISA, UMR CNRS 7583, Université Paris-Est-Créteil, Université de Paris, Institut Pierre Simon Laplace, Créteil, France.

Nilton Rennó (N)

Climate and Space Sciences and Engineering, University Michigan, Ann Arbor, United States.

John Rummel (J)

SETI Institute, Mountain View, United States.

Mitchell Schulte (M)

Science Mission Directorate, NASA HQ, Washington DC, United States.

Andrew Spry (A)

SETI Institute, Mountain View, United States.

Pericles Stabekis (P)

Retired, Gaithersburg, United States.

Alian Wang (A)

Department of Earth and Planetary Sciences, Washington University, St. Louis, United States.

Nathan Yee (N)

Department of Environmental Sciences, Rutgers University, Piscataway, United States.

Articles similaires

Calcium Carbonate Sand Powders Construction Materials Materials Testing
Cannabis Pakistan Phenotype Climate Geography

Experimental elevated temperature affects bumblebee foraging and flight speed.

Maxence Gérard, Erika Gardelin, Philipp Lehmann et al.
1.00
Animals Bees Flight, Animal Feeding Behavior Flowers

Classifications MeSH