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

Author

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., 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, A.-C., 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, C.L., Mance, D., Euchner, F., Kerjean, L., Mainsant, G., Mocquet, A., Rodriguez Manfredi, J. A, Pont, G., Laudet, P., Nebut, T., de Raucourt, S., Robert, O., Russell, C. T., Sylvestre-Baron, A., Tillier, S., Warren, T., Wieczorek, M., Yana, C., and Zweifel, P.

Published
2020
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2. Planetary Seismology: Nearly 3 years on Mars, and a return to the Moon

Author

Yana, Charles, Weber, Renee, Walsh, William, Standley, Ian, de Raucourt, Sebastien, Pont, Gabriel, Pike, W. Tom, Nunn, Ceri, Lognonné, Philippe, Kawamura, Taichi, Garcia, Raphael, Elliott, John, Cutler, James, Calcutt, Simon, Bugby, David, Bowles, Neil, Kedar, Sharon, Tharimena, S, Tauzin, B, Stutzmann, E, Schimmel, M, Schmelzbach, C, Nunn, C, Murdoch, N, Lekic, V, Brinkman, N, Kenda, B, Fayon, L, Spiga, A, Stott, A. E, Stähler, S, Orhand-Mainsant, G, Knapmeyer, M, Khan, A, Horleston, A, van Driel, M, Charalambous, C, Ceylan, S, Böse, M, Drilleau, M, Hurst, K, Weber, R, Teanby, N, Schmerr, N, Mimoun, D, Margerin, L, Knapmeyer-Endrun, B, Kedar, S, Kawamura, T, Irving, J, Garcia, R, Clinton, J, Bozdag, E, Lorenz, R, Giardini, D, Pike, W.T, Lognonné, P, Banerdt, W.B, and Panning, Mark

Published
2021

3. Planetary Seismology: Nearly 3 years on Mars, and a return to the Moon

Author

Panning, Mark, Banerdt, W.B, Lognonné, P, Pike, W.T, Giardini, D, Lorenz, R, Bozdag, E, Clinton, J, Garcia, R, Irving, J, Kawamura, T, Kedar, S, Knapmeyer-Endrun, B, Margerin, L, Mimoun, D, Schmerr, N, Teanby, N, Weber, R, Hurst, K, Drilleau, M, Böse, M, Ceylan, S, Charalambous, C, van Driel, M, Horleston, A, Khan, A, Knapmeyer, M, Orhand-Mainsant, G, Stähler, S, Stott, A. E, Spiga, A, Fayon, L, Kenda, B, Brinkman, N, Lekic, V, Murdoch, N, Nunn, C, Schmelzbach, C, Schimmel, M, Stutzmann, E, Tauzin, B, Tharimena, S, Kedar, Sharon, Bowles, Neil, Bugby, David, Calcutt, Simon, Cutler, James, Elliott, John, Garcia, Raphael, Kawamura, Taichi, Lognonné, Philippe, Nunn, Ceri, Pike, W. Tom, Pont, Gabriel, de Raucourt, Sebastien, Standley, Ian, Walsh, William, Weber, Renee, and Yana, Charles

Published
2021

4. SEIS: Insight’s Seismic Experiment for Internal Structure of Mars

Author

Lognonné, P., Banerdt, W. B., Giardini, D., Pike, W. T., Christensen, U., Laudet, P., de Raucourt, S., Zweifel, P., Calcutt, S., Bierwirth, M., Hurst, K. J., Ijpelaan, F., Umland, J. W., Llorca-Cejudo, R., Larson, S. A., Garcia, R. F., Kedar, S., Knapmeyer-Endrun, B., Mimoun, D., Mocquet, A., Panning, M. P., Weber, R. C., Sylvestre-Baron, A., Pont, G., Verdier, N., Kerjean, L., Facto, L. J., Gharakanian, V., Feldman, J. E., Hoffman, T. L., Klein, D. B., Klein, K., Onufer, N. P., Paredes-Garcia, J., Petkov, M. P., Willis, J. R., Smrekar, S. E., Drilleau, M., Gabsi, T., Nebut, T., Robert, O., Tillier, S., Moreau, C., Parise, M., Aveni, G., Ben Charef, S., Bennour, Y., Camus, T., Dandonneau, P. A., Desfoux, C., Lecomte, B., Pot, O., Revuz, P., Mance, D., tenPierick, J., Bowles, N. E., Charalambous, C., Delahunty, A. K., Hurley, J., Irshad, R., Liu, Huafeng, Mukherjee, A. G., Standley, I. M., Stott, A. E., Temple, J., Warren, T., Eberhardt, M., Kramer, A., Kühne, W., Miettinen, E.-P., Monecke, M., Aicardi, C., André, M., Baroukh, J., Borrien, A., Bouisset, A., Boutte, P., Brethomé, K., Brysbaert, C., Carlier, T., Deleuze, M., Desmarres, J. M., Dilhan, D., Doucet, C., Faye, D., Faye-Refalo, N., Gonzalez, R., Imbert, C., Larigauderie, C., Locatelli, E., Luno, L., Meyer, J.-R., Mialhe, F., Mouret, J. M., Nonon, M., Pahn, Y., Paillet, A., Pasquier, P., Perez, G., Perez, R., Perrin, L., Pouilloux, B., Rosak, A., Savin de Larclause, I., Sicre, J., Sodki, M., Toulemont, N., Vella, B., Yana, C., Alibay, F., Avalos, O. M., Balzer, M. A., Bhandari, P., Blanco, E., Bone, B. D., Bousman, J. C., Bruneau, P., Calef, F. J., Calvet, R. J., D’Agostino, S. A., de los Santos, G., Deen, R. G., Denise, R. W., Ervin, J., Ferraro, N. W., Gengl, H. E., Grinblat, F., Hernandez, D., Hetzel, M., Johnson, M. E., Khachikyan, L., Lin, J. Y., Madzunkov, S. M., Marshall, S. L., Mikellides, I. G., Miller, E. A., Raff, W., Singer, J. E., Sunday, C. M., Villalvazo, J. F., Wallace, M. C., Banfield, D., Rodriguez-Manfredi, J. A., Russell, C. T., Trebi-Ollennu, A., Maki, J. N., Beucler, E., Böse, M., Bonjour, C., Berenguer, J. L., Ceylan, S., Clinton, J., Conejero, V., Daubar, I., Dehant, V., Delage, P., Euchner, F., Estève, I., Fayon, L., Ferraioli, L., Johnson, C. L., Gagnepain-Beyneix, J., Golombek, M., Khan, A., Kawamura, T., Kenda, B., Labrot, P., Murdoch, N., Pardo, C., Perrin, C., Pou, L., Sauron, A., Savoie, D., Stähler, S., Stutzmann, E., Teanby, N. A., Tromp, J., van Driel, M., Wieczorek, M., Widmer-Schnidrig, R., and Wookey, J.

Published
2019
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5. Geology and Physical Properties Investigations by the InSight Lander

Author

Golombek, M., Grott, M., Kargl, G., Andrade, J., Marshall, J., Warner, N., Teanby, N. A., Ansan, V., Hauber, E., Voigt, J., Lichtenheldt, R., Knapmeyer-Endrun, B., Daubar, I. J., Kipp, D., Muller, N., Lognonné, P., Schmelzbach, C., Banfield, D., Trebi-Ollennu, A., Maki, J., Kedar, S., Mimoun, D., Murdoch, N., Piqueux, S., Delage, P., Pike, W. T., Charalambous, C., Lorenz, R., Fayon, L., Lucas, A., Rodriguez, S., Morgan, P., Spiga, A., Panning, M., Spohn, T., Smrekar, S., Gudkova, T., Garcia, R., Giardini, D., Christensen, U., Nicollier, T., Sollberger, D., Robertsson, J., Ali, K., Kenda, B., and Banerdt, W. B.

Published
2018
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6. The Polarization of Ambient Noise on Mars

Author

Agence Nationale de la Recherche (France), UK Space Agency, Ministerio de Ciencia, Innovación y Universidades (España), Schimmel, Martin [0000-0003-2601-4462], Stutzmann, E., Schimmel, Martin, Lognonné, P., Horleston, A., Ceylan, S., van Driel, M., Stähler, S., Banerdt, B., Calvet, M., Charalambous, C., Clinton, John F., Drilleau, M., Fayon, L., Garcia, R. F., Giardini, Domenico, Hurst, K., Jacob, A., Kawamura, T., Kenda, B., Margerin, L., Murdoch, N., Panning, M., Pike, T., Scholz, J. R., Spiga, A., Agence Nationale de la Recherche (France), UK Space Agency, Ministerio de Ciencia, Innovación y Universidades (España), Schimmel, Martin [0000-0003-2601-4462], Stutzmann, E., Schimmel, Martin, Lognonné, P., Horleston, A., Ceylan, S., van Driel, M., Stähler, S., Banerdt, B., Calvet, M., Charalambous, C., Clinton, John F., Drilleau, M., Fayon, L., Garcia, R. F., Giardini, Domenico, Hurst, K., Jacob, A., Kawamura, T., Kenda, B., Margerin, L., Murdoch, N., Panning, M., Pike, T., Scholz, J. R., and Spiga, A.

Abstract

Seismic noise recorded at the surface of Mars has been monitored since February 2019, using the InSight seismometers. This noise can reach -200 dB. It is 500 times lower than on Earth at night and it increases of 30 dB during the day. We analyze its polarization as a function of time and frequency in the band 0.03-1 Hz. We use the degree of polarization to extract signals with stable polarization independent of their amplitude and type of polarization. We detect polarized signals at all frequencies and all times. Glitches correspond to linear polarized signals which are more abundant during the night. For signals with elliptical polarization, the ellipse is in the horizontal plane below 0.3 Hz. In the 0.3-1Hz high frequency band (HF) and except in the evening, the ellipse is in the vertical plane and the major axis is tilted. While polarization azimuths are different in the two frequency bands, they both vary as a function of local hour and season. They are also correlated with wind direction, particularly during the daytime. We investigate possible aseismic and seismic origins of the polarized signals. Lander or tether noise can be discarded. Pressure fluctuations transported by wind may explain part of the HF polarization but not the tilt of the ellipse. This tilt can be obtained if the source is an acoustic emission coming from high altitude at critical angle. Finally, in the evening when the wind is low, the measured polarized signals may correspond to the seismic wavefield of the Mars background noise. Plain Language Summary Seismic noise at the surface of Mars was unknown until the first measurements by the seismometers from the InSight mission in January 2019. On Earth, the microseismic noise (0.05-1 Hz) is composed dominantly of surface waves generated by the numerous sources related to ocean wave activities. On Mars, because there is no ocean, seismic noise is down to 500 times lower than on Earth reaching -200 dB in acceleration at night. In order to deter

Published
2021

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

Author

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.; 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.; Schimmel, M.; Rodriguez Manfredi, J.A. and 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.; 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.; Schimmel, M.; Rodriguez Manfredi, J.A.

Abstract

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 (HP) 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.

Published
2020

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

Author

Centre National D'Etudes Spatiales (France), California Institute of Technology, NASA Astrobiology Institute (US), Swiss National Science Foundation, European Commission, Schimmel, Martin [0000-0003-2601-4462], Lognonné, P., Banerdt, W. B., Pike, William T., Giardini, Domenico, Christensen, U., Garcia, R. F., Kawamura, T., Kedar, S., Knapmeyer‐Endrun, Brigitte, Margerin, L., Nimmo, F., 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, Robert, Nissen-Meyer, T., ten Pierick, J., Plesa, A. C., Quantin-Nataf, C., Robertsson, J., Rochas, L., Schimmel, Martin, 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, C. L., Mance, D., Euchner, F., Kerjean, L., Mainsant, G., Mocquet, A., Rodriguez Manfredi, J. A., Pont, G., Laudet, P., Nebut, T., de Raucourt, S., Robert, O., Russell, C. T., Sylvestre-Baron, A., Tillier, S., Warren, T., Wieczorek, M., Yana, C., Zweifel, P., Panning, M., Tauzin, B., Scholz, J. R., 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, Vedran, McClean, J., Mimoun, D., Murdoch, N., Pan, L., Perrin , C., Pinot, B, Pou, L., Menina, S., Rodríguez, 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, John F., Centre National D'Etudes Spatiales (France), California Institute of Technology, NASA Astrobiology Institute (US), Swiss National Science Foundation, European Commission, Schimmel, Martin [0000-0003-2601-4462], Lognonné, P., Banerdt, W. B., Pike, William T., Giardini, Domenico, Christensen, U., Garcia, R. F., Kawamura, T., Kedar, S., Knapmeyer‐Endrun, Brigitte, Margerin, L., Nimmo, F., 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, Robert, Nissen-Meyer, T., ten Pierick, J., Plesa, A. C., Quantin-Nataf, C., Robertsson, J., Rochas, L., Schimmel, Martin, 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, C. L., Mance, D., Euchner, F., Kerjean, L., Mainsant, G., Mocquet, A., Rodriguez Manfredi, J. A., Pont, G., Laudet, P., Nebut, T., de Raucourt, S., Robert, O., Russell, C. T., Sylvestre-Baron, A., Tillier, S., Warren, T., Wieczorek, M., Yana, C., Zweifel, P., Panning, M., Tauzin, B., Scholz, J. R., 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, Vedran, McClean, J., Mimoun, D., Murdoch, N., Pan, L., Perrin , C., Pinot, B, Pou, L., Menina, S., Rodríguez, 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., and Clinton, John F.

Abstract

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.

Published
2020

9. The Polarization of Ambient Noise on Mars

Author

Stutzmann, E., primary, Schimmel, M., additional, Lognonné, P., additional, Horleston, A., additional, Ceylan, S., additional, van Driel, M., additional, Stahler, S., additional, Banerdt, B., additional, Calvet, M., additional, Charalambous, C., additional, Clinton, J., additional, Drilleau, M., additional, Fayon, L., additional, Garcia, R. F., additional, Giardini, D., additional, Hurst, K., additional, Jacob, A., additional, Kawamura, T., additional, Kenda, B., additional, Margerin, L., additional, Murdoch, N., additional, Panning, M., additional, Pike, T., additional, Scholz, J.‐R., additional, and Spiga, A., additional

Published
2021
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10. Characterization of the InSight Landing Site near Surface Properties using the Heat Flow and Physical Properties Probe (HP3) mole as a Seismic Source

Author

Kedar, S., Banerdt, W.B., Brinkmann, Nienke, Charalambous, C., Delage, P., Fayon, L., Gaudin, E., Giardini, D., Grott, Matthias, Horleston, A., Hudson, T.L., Hurst, K., Kiely, A., Kerjean, L, Knapmeyer-Endrun, B., Krasner, S., Krause, Christian, Lognonne, P., McLean, J., Nonon, M., Pike, T., Robertsson, J., Schmelzbach, C., Schmerr, N., Stott, A.E., Spohn, Tilman, Sollberger, D., Stähler, S., Teanby, N., Vallade, J., van Driel, M, Verdier, N, Vrettos, C., Warren, T., Widmer-Schnidrig, Rudolf, and Yana, Charles

Subjects
InSight Mars Geophysics HP3
Published
2019

11. Extraterrestrial Seismology: The Perspective After Nearly 1 Year of InSight on Mars

Author

Panning, M., Banerdt, B., Lognonne, P., Pike, W.T., Giardini, D., Lorenz, R. D., Bozdag, E., Clinton, J., Garcia, R., Irving, J., Kawamura, T., Kedar, S., Knapmeyer-Endrun, B., Margerin, L., Mimoun, D., Schmerr, N., Teanby, N., Weber, R., Hurst, K., Drilleau, M., Böse, M, Ceylan, S., Charalambous, C., van Driel, M, Horleston, A., Khan, A., Knapmeyer, Martin, Orhand-Mainsant, G., Stähler, S., Stott, A.E., Spiga, Aymeric, Fayon, L., Kenda, B., Brinkmann, Nienke, Lekic, V., Murdoch, N., Nunn, C., Schmelzbach, C., Schimmel, M., Stutzmann, Éléonore, Tauzin, B., and Tharimena, S.

Subjects
Mars, Seismology, InSight
Published
2019

12. SEIS: Overview, Deployment, and First Science on the Ground

Author

Lognonné, P., Banerdt, W. B., Pike, W. T., Giardini, Domenico, Banfield, D., Christensen, U., Bierwirth, M., S. Calcutt, S., Clinton, John F., Kedar, S., Garcia, R., de Raucourt, S., Hurst, K., Kawamura, T., Mimoun, D., Panning, M., Spiga, A., Zweifel, P., Beucler, E., Verdier, N. Ceylan, S., Charalambous, C., Drilleau, M., Eberhardt, M., Fayon, L., Gabsi, T., Kenda, B., Kramer, A., Mainsant, G., Mance, D., McClean, J., Murdoch, N., Nebut, T., Pardo, C., Perrin, C., Robert, O., Savoie, D., Schimmel, Martin, Stähler, S., Stutzmann, E., Stott, A., Ten Pierick, J., Tillier, S., van Driel, M., Warren, T., and Widmer-Schnidrig, R.

Subjects
Mars, The InSight mission
Abstract

The 50th Lunar and Planetary Science Conference in The Woodlands, Texas, March 18–22, 2019., Introduction: The InSight mission landed on Mars on November, 26, 2018. This is the first planetary mission designed to deploy a complete geophysical observatory on Mars, following in the footsteps of the Apollo Lunar Surface Experiments Package (ALSEP) deployed on the Moon in the 1970s [1]. It will thus provide the first ground truth constraints on interior structure of the planet. The Seismic Experiment for Interior Structure (SEIS) [2] is one of three primary scientific investigations, the others being the Heat Flow and Physical Properties Package (HP3) [3] and the Rotation and Interior Structure Experiment (RISE) [4]. SEIS is supported by the APSS package, (Auxiliary Payload Sensor Suite, [5]), whose goal is to document environmental sources of seismic noise and signals, as well as an imaging system [6]. After a brief description of the SEIS experiment, we will describe the deployment process, including the evolution of the SEIS noise from the deck (with only SPs) to the ground (with both VBBs and SPs), first without and finally with wind shield. We will then discuss early scientific observations, providing first constrains on the Mars micro-seismic noise, atmospherically-generated seismic signals, and surface and subsurface elastic structure., The SEIS team acknowledge the supports of NASA, CNES, UKSA, SSO and DLR for the experiment funding and of the SEIS operation team [38] for delivering SEIS data.

Published
2019

13. Characterization of the InSight Near Surface Seismic Properites using the Heat Flow and Physical Properties Probe (HP3) Mole as a Seismic Source

Author

Kedar, S., Banerdt, B., Brinkmann, Nienke, Delage, P., Fayon, L., Grott, M, Horleston, A., Hudson, T.L., Hurst, K., Kiely, A., Knapmeyer-Endrun, B., Krause, Christian, Lognonne, P., Pike, W.T., Robertsson, J., Schmelzbach, C., Schmerr, N., Spohn, Tilman, Solberger, D., Stähler, S., Teanby, N., van Driel, M, and Vrettos, C.

Subjects
Planetenphysik, Seismicity, HP3, Leitungsbereich PF, Mars, InSight, Nutzerzentrum für Weltraumexperimente (MUSC)
Published
2019

14. Seismic near-surface investigations at the InSight landing site using the Heat and Physical Properties (HP3) probe as a seismic source

Author

Schmelzbach, C., Banerdt, B., Brinkmann, Nienke, Fayon, L., Grott, Matthias, Horleston, A., Hudson, T.L., Hurst, K., Kedar, S., Kiely, A., Knapmeyer-Endrun, B., Krause, Christian, Lognonne, A.P., Pike, W.T., Robertsson, J., Schmerr, N., Sollberger, D., Spohn, Tilman, Teanby, N., and van Driel, M

Subjects
Planetenphysik, Geophysik, HP3, Leitungsbereich PF, Mars, Seismologie, InSight, Nutzerzentrum für Weltraumexperimente (MUSC)
Published
2019

15. The first active seismic experiment on Mars to characterize the shallow subsurface structure at the InSight landing site

Author

Brinkman, N., primary, Schmelzbach, C., additional, Sollberger, D., additional, van Driel, M., additional, ten Pierick, J., additional, Robertsson, J. O. A., additional, Andersson, F., additional, Stähler, S., additional, Giardini, D., additional, Kedar, S., additional, Hudson, T., additional, Hurst, K., additional, KiVely, A., additional, Banerdt, W. B., additional, Grott, M., additional, Spohn, T., additional, Krause, C., additional, Fayon, L., additional, Lognonné, P., additional, Knapmeyer-Endrun, B., additional, Delage, P., additional, Pike, W. T., additional, Horleston, A., additional, Teanby, N., additional, and Vretto, C., additional

Published
2019
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