Imperial College London
Portrait Picture

Professor Tom Pike

Faculty of Engineering, Department of Electrical and Electronic Engineering

Professor of Microengineering
 
 
 
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Contact

 

+44 (0)20 7594 6207w.t.pike

 
 
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Location

 

604Electrical EngineeringSouth Kensington Campus

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Summary

 

Publications

Citation

BibTex format

@article{Posiolova:2022:10.1126/science.abq7704,
author = {Posiolova, LV and Lognonné, P and Banerdt, WB and Clinton, J and Collins, GS and Kawamura, T and Ceylan, S and Daubar, IJ and Fernando, B and Froment, M and Giardini, D and Malin, MC and Miljkovi, K and Stähler, SC and Xu, Z and Banks, ME and Beucler, É and Cantor, BA and Charalambous, C and Dahmen, N and Davis, P and Drilleau, M and Dundas, CM and Durán, C and Euchner, F and Garcia, RF and Golombek, M and Horleston, A and Keegan, C and Khan, A and Kim, D and Larmat, C and Lorenz, R and Margerin, L and Menina, S and Panning, M and Pardo, C and Perrin, C and Pike, WT and Plasman, M and Raji, A and Rolland, L and Rougier, E and Speth, G and Spiga, A and Stott, A and Susko, D and Teanby, NA and Valeh, A and Werynski, A and Wójcicka, N and Zenhäusern, G},
doi = {10.1126/science.abq7704},
journal = {Science},
pages = {412--417},
title = {Largest recent impact craters on Mars: Orbital imaging and surface seismic co-investigation.},
url = {http://dx.doi.org/10.1126/science.abq7704},
volume = {378},
year = {2022}
}
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RIS format (EndNote, RefMan)

TY  - JOUR
AB  - Two >130-meter-diameter impact craters formed on Mars during the later half of 2021. These are the two largest fresh impact craters discovered by the Mars Reconnaissance Orbiter since operations started 16 years ago. The impacts created two of the largest seismic events (magnitudes greater than 4) recorded by InSight during its 3-year mission. The combination of orbital imagery and seismic ground motion enables the investigation of subsurface and atmospheric energy partitioning of the impact process on a planet with a thin atmosphere and the first direct test of martian deep-interior seismic models with known event distances. The impact at 35°N excavated blocks of water ice, which is the lowest latitude at which ice has been directly observed on Mars.
AU  - Posiolova,LV
AU  - Lognonné,P
AU  - Banerdt,WB
AU  - Clinton,J
AU  - Collins,GS
AU  - Kawamura,T
AU  - Ceylan,S
AU  - Daubar,IJ
AU  - Fernando,B
AU  - Froment,M
AU  - Giardini,D
AU  - Malin,MC
AU  - Miljkovi,K
AU  - Stähler,SC
AU  - Xu,Z
AU  - Banks,ME
AU  - Beucler,É
AU  - Cantor,BA
AU  - Charalambous,C
AU  - Dahmen,N
AU  - Davis,P
AU  - Drilleau,M
AU  - Dundas,CM
AU  - Durán,C
AU  - Euchner,F
AU  - Garcia,RF
AU  - Golombek,M
AU  - Horleston,A
AU  - Keegan,C
AU  - Khan,A
AU  - Kim,D
AU  - Larmat,C
AU  - Lorenz,R
AU  - Margerin,L
AU  - Menina,S
AU  - Panning,M
AU  - Pardo,C
AU  - Perrin,C
AU  - Pike,WT
AU  - Plasman,M
AU  - Raji,A
AU  - Rolland,L
AU  - Rougier,E
AU  - Speth,G
AU  - Spiga,A
AU  - Stott,A
AU  - Susko,D
AU  - Teanby,NA
AU  - Valeh,A
AU  - Werynski,A
AU  - Wójcicka,N
AU  - Zenhäusern,G
DO  - 10.1126/science.abq7704
EP  - 417
PY  - 2022///
SN  - 0036-8075
SP  - 412
TI  - Largest recent impact craters on Mars: Orbital imaging and surface seismic co-investigation.
T2  - Science
UR  - http://dx.doi.org/10.1126/science.abq7704
UR  - https://www.ncbi.nlm.nih.gov/pubmed/36302013
UR  - https://www.science.org/doi/10.1126/science.abq7704
UR  - http://hdl.handle.net/10044/1/100459
VL  - 378
ER  -
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