Constraints on the shallow elastic and anelastic structure of Mars from InSight seismic data

P. Lognonné; W. B. Banerdt; W. T. Pike; D. Giardini; U. Christensen; R. F. Garcia; T. Kawamura; S. Kedar; B. Knapmeyer-Endrun; L. Margerin; F. Nimmo; M. Panning; B. Tauzin; J. R. Scholz; D. Antonangeli; S. Barkaoui; E. Beucler; F. Bissig; N. Brinkman; M. Calvet; S. Ceylan; C. Charalambous; P. Davis; M. van Driel; M. Drilleau; L. Fayon; R. Joshi; B. Kenda; A. Khan; M. Knapmeyer; V. Lekic; J. McClean; D. Mimoun; N. Murdoch; L. Pan; C. Perrin; B. Pinot; L. Pou; S. Menina; S. Rodriguez; C. Schmelzbach; N. Schmerr; D. Sollberger; A. Spiga; S. Stähler; A. Stott; E. Stutzmann; S. Tharimena; R. Widmer-Schnidrig; F. Andersson; V. Ansan; C. Beghein; M. Böse; E. Bozdag; J. Clinton; I. Daubar; P. Delage; N. Fuji; M. Golombek; M. Grott; A. Horleston; K. Hurst; J. Irving; A. Jacob; J. Knollenberg; S. Krasner; C. Krause; R. Lorenz; C. Michaut; R. Myhill; T. Nissen-Meyer; J. ten Pierick; A. C. Plesa; C. Quantin-Nataf; J. Robertsson; L. Rochas; M. Schimmel; S. Smrekar; T. Spohn; N. Teanby; J. Tromp; J. Vallade; N. Verdier; C. Vrettos; R. Weber; D. Banfield; E. Barrett; M. Bierwirth; S. Calcutt; N. Compaire; C. L. Johnson; D. Mance; F. Euchner; L. Kerjean; G. Mainsant; A. Mocquet; J. A. Rodriguez Manfredi; G. Pont; P. Laudet; T. Nebut; S. de Raucourt; O. Robert; C. T. Russell; A. Sylvestre-Baron; S. Tillier; T. Warren; M. Wieczorek; C. Yana; P. Zweifel

doi:10.1038/s41561-020-0536-y

Constraints on the shallow elastic and anelastic structure of Mars from InSight seismic data

P. Lognonné^*
, W. B. Banerdt
, W. T. Pike
, D. Giardini
, U. Christensen
, R. F. Garcia
, T. Kawamura
, S. Kedar
, B. Knapmeyer-Endrun
, L. Margerin
, F. Nimmo
, M. Panning
, B. Tauzin
, J. R. Scholz
, D. Antonangeli
, S. Barkaoui
, E. Beucler
, F. Bissig
, N. Brinkman
, M. Calvet

S. Ceylan, C. Charalambous, P. Davis, M. van Driel, M. Drilleau, L. Fayon, R. Joshi, B. Kenda, A. Khan, M. Knapmeyer, V. Lekic, J. McClean, D. Mimoun, N. Murdoch, L. Pan, C. Perrin, B. Pinot, L. Pou, S. Menina, S. Rodriguez, C. Schmelzbach, N. Schmerr, D. Sollberger, A. Spiga, S. Stähler, A. Stott, E. Stutzmann, S. Tharimena, R. Widmer-Schnidrig, F. Andersson, V. Ansan, C. Beghein, M. Böse, E. Bozdag, J. Clinton, I. Daubar, P. Delage, N. Fuji, M. Golombek, M. Grott, A. Horleston, K. Hurst, J. Irving, A. Jacob, J. Knollenberg, S. Krasner, C. Krause, R. Lorenz, C. Michaut, R. Myhill, T. Nissen-Meyer, J. ten Pierick, A. C. Plesa, C. Quantin-Nataf, J. Robertsson, L. Rochas, M. Schimmel, S. Smrekar, T. Spohn, N. Teanby, J. Tromp, J. Vallade, N. Verdier, C. Vrettos, R. Weber, D. Banfield, E. Barrett, M. Bierwirth, S. Calcutt, N. Compaire, C. L. Johnson, D. Mance, F. Euchner, L. Kerjean, G. Mainsant, A. Mocquet, J. A. Rodriguez Manfredi, G. Pont, P. Laudet, T. Nebut, S. de Raucourt, O. Robert, C. T. Russell, A. Sylvestre-Baron, S. Tillier, T. Warren, M. Wieczorek, C. Yana, P. Zweifel

^*Bu çalışma için yazışmadan sorumlu yazar

Université Paris Cité
Institut universitaire de France
Jet Propulsion Laboratory, California Institute of Technology
Imperial College London
Swiss Federal Institute of Technology Zurich
Max Planck Institute for Solar System Research
Université Fédérale Toulouse Midi-Pyrénées
University of Cologne
Centre d'Etude Spatiale des Rayonnements
University of California at Santa Cruz
Universite Claude Bernard Lyon 1
Sorbonne Université
Nantes Université
University of California at Los Angeles
Space Exploration Institute
University of Zurich
German Aerospace Center
University of Maryland, College Park
Ecole Normale Supérieure
University of Stuttgart
Colorado School of Mines
CNRS
University of Bristol
Princeton University
Johns Hopkins University Applied Physics Laboratory
École normale supérieure de Lyon
University of Oxford
Centre National d’Etudes Spatiales
ICTJA-CSIC
International Space Science Institute
Technical University of Kaiserslautern
NASA Marshall Space Flight Center
Cornell University
University of British Columbia
Planetary Science Institute
Instituto Nacional de Tecnica Aeroespacial
Université Côte d'Azur

Araştırma sonucu: Dergiye katkı › Makale › bilirkişi

275 Atıf (Scopus)

Özet

Mars’s seismic activity and noise have been monitored since January 2019 by the seismometer of the InSight (Interior Exploration using Seismic Investigations, Geodesy and Heat Transport) lander. At night, Mars is extremely quiet; seismic noise is about 500 times lower than Earth’s microseismic noise at periods between 4 s and 30 s. The recorded seismic noise increases during the day due to ground deformations induced by convective atmospheric vortices and ground-transferred wind-generated lander noise. Here we constrain properties of the crust beneath InSight, using signals from atmospheric vortices and from the hammering of InSight’s Heat Flow and Physical Properties (HP³) instrument, as well as the three largest Marsquakes detected as of September 2019. From receiver function analysis, we infer that the uppermost 8–11 km of the crust is highly altered and/or fractured. We measure the crustal diffusivity and intrinsic attenuation using multiscattering analysis and find that seismic attenuation is about three times larger than on the Moon, which suggests that the crust contains small amounts of volatiles.

Orijinal dil	İngilizce
Sayfa (başlangıç-bitiş)	213-220
Sayfa sayısı	8
Dergi	Nature Geoscience
Hacim	13
Basın numarası	3
DOI'lar	https://doi.org/10.1038/s41561-020-0536-y
Yayın durumu	Yayınlandı - 1 Mar 2020
Harici olarak yayınlandı	Evet

Bibliyografik not

Publisher Copyright:
© 2020, The Author(s), under exclusive licence to Springer Nature Limited.

Belgeye Erişim

10.1038/s41561-020-0536-y

Diğer Dosyalar ve Linkler

Link to publication in Scopus

Alıntı Yap

Lognonné, P., Banerdt, W. B., Pike, W. T., Giardini, D., Christensen, U., Garcia, R. F., Kawamura, T., Kedar, S., Knapmeyer-Endrun, B., Margerin, L., Nimmo, F., Panning, M., Tauzin, B., Scholz, J. R., Antonangeli, D., Barkaoui, S., Beucler, E., Bissig, F., Brinkman, N., ... Zweifel, P. (2020). Constraints on the shallow elastic and anelastic structure of Mars from InSight seismic data. Nature Geoscience, 13(3), 213-220. https://doi.org/10.1038/s41561-020-0536-y

@article{20ed7193b06a4a418a0e3cd3d80c7b69,

title = "Constraints on the shallow elastic and anelastic structure of Mars from InSight seismic data",

abstract = "Mars{\textquoteright}s seismic activity and noise have been monitored since January 2019 by the seismometer of the InSight (Interior Exploration using Seismic Investigations, Geodesy and Heat Transport) lander. At night, Mars is extremely quiet; seismic noise is about 500 times lower than Earth{\textquoteright}s microseismic noise at periods between 4 s and 30 s. The recorded seismic noise increases during the day due to ground deformations induced by convective atmospheric vortices and ground-transferred wind-generated lander noise. Here we constrain properties of the crust beneath InSight, using signals from atmospheric vortices and from the hammering of InSight{\textquoteright}s Heat Flow and Physical Properties (HP3) instrument, as well as the three largest Marsquakes detected as of September 2019. From receiver function analysis, we infer that the uppermost 8–11 km of the crust is highly altered and/or fractured. We measure the crustal diffusivity and intrinsic attenuation using multiscattering analysis and find that seismic attenuation is about three times larger than on the Moon, which suggests that the crust contains small amounts of volatiles.",

author = "P. Lognonn{\'e} and Banerdt, \{W. B.\} and Pike, \{W. T.\} and D. Giardini and U. Christensen and Garcia, \{R. F.\} and T. Kawamura and S. Kedar and B. Knapmeyer-Endrun and L. Margerin and F. Nimmo and M. Panning and B. Tauzin and Scholz, \{J. R.\} and D. Antonangeli and S. Barkaoui and E. Beucler and F. Bissig and N. Brinkman and M. Calvet and S. Ceylan and C. Charalambous and P. Davis and \{van Driel\}, M. and M. Drilleau and L. Fayon and R. Joshi and B. Kenda and A. Khan and M. Knapmeyer and V. Lekic and J. McClean and D. Mimoun and N. Murdoch and L. Pan and C. Perrin and B. Pinot and L. Pou and S. Menina and S. Rodriguez and C. Schmelzbach and N. Schmerr and D. Sollberger and A. Spiga and S. St{\"a}hler and A. Stott and E. Stutzmann and S. Tharimena and R. Widmer-Schnidrig and F. Andersson and V. Ansan and C. Beghein and M. B{\"o}se and E. Bozdag and J. Clinton and I. Daubar and P. Delage and N. Fuji and M. Golombek and M. Grott and A. Horleston and K. Hurst and J. Irving and A. Jacob and J. Knollenberg and S. Krasner and C. Krause and R. Lorenz and C. Michaut and R. Myhill and T. Nissen-Meyer and \{ten Pierick\}, J. and Plesa, \{A. C.\} and C. Quantin-Nataf and J. Robertsson and L. Rochas and M. Schimmel and S. Smrekar and T. Spohn and N. Teanby and J. Tromp and J. Vallade and N. Verdier and C. Vrettos and R. Weber and D. Banfield and E. Barrett and M. Bierwirth and S. Calcutt and N. Compaire and Johnson, \{C. L.\} and D. Mance and F. Euchner and L. Kerjean and G. Mainsant and A. Mocquet and \{Rodriguez Manfredi\}, \{J. A.\} and G. Pont and P. Laudet and T. Nebut and \{de Raucourt\}, S. and O. Robert and Russell, \{C. T.\} and A. Sylvestre-Baron and S. Tillier and T. Warren and M. Wieczorek and C. Yana and P. Zweifel",

note = "Publisher Copyright: {\textcopyright} 2020, The Author(s), under exclusive licence to Springer Nature Limited.",

year = "2020",

month = mar,

day = "1",

doi = "10.1038/s41561-020-0536-y",

language = "English",

volume = "13",

pages = "213--220",

journal = "Nature Geoscience",

issn = "1752-0894",

publisher = "Nature Publishing Group",

number = "3",

}

Lognonné, P, Banerdt, WB, Pike, WT, Giardini, D, Christensen, U, Garcia, RF, Kawamura, T, Kedar, S, Knapmeyer-Endrun, B, Margerin, L, Nimmo, F, Panning, M, Tauzin, B, Scholz, JR, Antonangeli, D, Barkaoui, S, Beucler, E, Bissig, F, Brinkman, N, Calvet, M, Ceylan, S, Charalambous, C, Davis, P, van Driel, M, Drilleau, M, Fayon, L, Joshi, R, Kenda, B, Khan, A, Knapmeyer, M, Lekic, V, McClean, J, Mimoun, D, Murdoch, N, Pan, L, Perrin, C, Pinot, B, Pou, L, Menina, S, Rodriguez, S, Schmelzbach, C, Schmerr, N, Sollberger, D, Spiga, A, Stähler, S, Stott, A, Stutzmann, E, Tharimena, S, Widmer-Schnidrig, R, Andersson, F, Ansan, V, Beghein, C, Böse, M, Bozdag, E, Clinton, J, Daubar, I, Delage, P, Fuji, N, Golombek, M, Grott, M, Horleston, A, Hurst, K, Irving, J, Jacob, A, Knollenberg, J, Krasner, S, Krause, C, Lorenz, R, Michaut, C, Myhill, R, Nissen-Meyer, T, ten Pierick, J, Plesa, AC, Quantin-Nataf, C, Robertsson, J, Rochas, L, Schimmel, M, Smrekar, S, Spohn, T, Teanby, N, Tromp, J, Vallade, J, Verdier, N, Vrettos, C, Weber, R, Banfield, D, Barrett, E, Bierwirth, M, Calcutt, S, Compaire, N, Johnson, CL, Mance, D, Euchner, F, Kerjean, L, Mainsant, G, Mocquet, A, Rodriguez Manfredi, JA, Pont, G, Laudet, P, Nebut, T, de Raucourt, S, Robert, O, Russell, CT, Sylvestre-Baron, A, Tillier, S, Warren, T, Wieczorek, M, Yana, C & Zweifel, P 2020, 'Constraints on the shallow elastic and anelastic structure of Mars from InSight seismic data', Nature Geoscience, hac. 13, no. 3, pp. 213-220. https://doi.org/10.1038/s41561-020-0536-y

TY - JOUR

T1 - Constraints on the shallow elastic and anelastic structure of Mars from InSight seismic data

AU - Lognonné, P.

AU - Banerdt, W. B.

AU - Pike, W. T.

AU - Giardini, D.

AU - Christensen, U.

AU - Garcia, R. F.

AU - Kawamura, T.

AU - Kedar, S.

AU - Knapmeyer-Endrun, B.

AU - Margerin, L.

AU - Nimmo, F.

AU - Panning, M.

AU - Tauzin, B.

AU - Scholz, J. R.

AU - Antonangeli, D.

AU - Barkaoui, S.

AU - Beucler, E.

AU - Bissig, F.

AU - Brinkman, N.

AU - Calvet, M.

AU - Ceylan, S.

AU - Charalambous, C.

AU - Davis, P.

AU - van Driel, M.

AU - Drilleau, M.

AU - Fayon, L.

AU - Joshi, R.

AU - Kenda, B.

AU - Khan, A.

AU - Knapmeyer, M.

AU - Lekic, V.

AU - McClean, J.

AU - Mimoun, D.

AU - Murdoch, N.

AU - Pan, L.

AU - Perrin, C.

AU - Pinot, B.

AU - Pou, L.

AU - Menina, S.

AU - Rodriguez, S.

AU - Schmelzbach, C.

AU - Schmerr, N.

AU - Sollberger, D.

AU - Spiga, A.

AU - Stähler, S.

AU - Stott, A.

AU - Stutzmann, E.

AU - Tharimena, S.

AU - Widmer-Schnidrig, R.

AU - Andersson, F.

AU - Ansan, V.

AU - Beghein, C.

AU - Böse, M.

AU - Bozdag, E.

AU - Clinton, J.

AU - Daubar, I.

AU - Delage, P.

AU - Fuji, N.

AU - Golombek, M.

AU - Grott, M.

AU - Horleston, A.

AU - Hurst, K.

AU - Irving, J.

AU - Jacob, A.

AU - Knollenberg, J.

AU - Krasner, S.

AU - Krause, C.

AU - Lorenz, R.

AU - Michaut, C.

AU - Myhill, R.

AU - Nissen-Meyer, T.

AU - ten Pierick, J.

AU - Plesa, A. C.

AU - Quantin-Nataf, C.

AU - Robertsson, J.

AU - Rochas, L.

AU - Schimmel, M.

AU - Smrekar, S.

AU - Spohn, T.

AU - Teanby, N.

AU - Tromp, J.

AU - Vallade, J.

AU - Verdier, N.

AU - Vrettos, C.

AU - Weber, R.

AU - Banfield, D.

AU - Barrett, E.

AU - Bierwirth, M.

AU - Calcutt, S.

AU - Compaire, N.

AU - Johnson, C. L.

AU - Mance, D.

AU - Euchner, F.

AU - Kerjean, L.

AU - Mainsant, G.

AU - Mocquet, A.

AU - Rodriguez Manfredi, J. A.

AU - Pont, G.

AU - Laudet, P.

AU - Nebut, T.

AU - de Raucourt, S.

AU - Robert, O.

AU - Russell, C. T.

AU - Sylvestre-Baron, A.

AU - Tillier, S.

AU - Warren, T.

AU - Wieczorek, M.

AU - Yana, C.

AU - Zweifel, P.

PY - 2020/3/1

Y1 - 2020/3/1

N2 - Mars’s seismic activity and noise have been monitored since January 2019 by the seismometer of the InSight (Interior Exploration using Seismic Investigations, Geodesy and Heat Transport) lander. At night, Mars is extremely quiet; seismic noise is about 500 times lower than Earth’s microseismic noise at periods between 4 s and 30 s. The recorded seismic noise increases during the day due to ground deformations induced by convective atmospheric vortices and ground-transferred wind-generated lander noise. Here we constrain properties of the crust beneath InSight, using signals from atmospheric vortices and from the hammering of InSight’s Heat Flow and Physical Properties (HP3) instrument, as well as the three largest Marsquakes detected as of September 2019. From receiver function analysis, we infer that the uppermost 8–11 km of the crust is highly altered and/or fractured. We measure the crustal diffusivity and intrinsic attenuation using multiscattering analysis and find that seismic attenuation is about three times larger than on the Moon, which suggests that the crust contains small amounts of volatiles.

AB - Mars’s seismic activity and noise have been monitored since January 2019 by the seismometer of the InSight (Interior Exploration using Seismic Investigations, Geodesy and Heat Transport) lander. At night, Mars is extremely quiet; seismic noise is about 500 times lower than Earth’s microseismic noise at periods between 4 s and 30 s. The recorded seismic noise increases during the day due to ground deformations induced by convective atmospheric vortices and ground-transferred wind-generated lander noise. Here we constrain properties of the crust beneath InSight, using signals from atmospheric vortices and from the hammering of InSight’s Heat Flow and Physical Properties (HP3) instrument, as well as the three largest Marsquakes detected as of September 2019. From receiver function analysis, we infer that the uppermost 8–11 km of the crust is highly altered and/or fractured. We measure the crustal diffusivity and intrinsic attenuation using multiscattering analysis and find that seismic attenuation is about three times larger than on the Moon, which suggests that the crust contains small amounts of volatiles.

UR - https://www.scopus.com/pages/publications/85079827100

U2 - 10.1038/s41561-020-0536-y

DO - 10.1038/s41561-020-0536-y

M3 - Article

AN - SCOPUS:85079827100

SN - 1752-0894

VL - 13

SP - 213

EP - 220

JO - Nature Geoscience

JF - Nature Geoscience

IS - 3

ER -

Constraints on the shallow elastic and anelastic structure of Mars from InSight seismic data

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