Little is known of the internal structure or composition of Mars or the present rates and characteristics of tectonic activity and meteoroid impacts. The scientific tool best suited to address these issues is seismology. While a simple seismic experiment was included on the two Viking landers, one of the instruments did not operate and the experiment was severely limited by the location of the sensor high on the lander, the low sensitivity of the instrument, and the limited data rate allocated to seismic measurements
International audienceThe study of the deep interior of Mars suffers from the very limited amount of...
Our fundamental understanding of the interior of the Earth comes from seismology, geodesy, geochemis...
none24siOur fundamental understanding of the interior of the Earth comes from seismology, geodesy, g...
Little is known of the internal structure or composition of Mars or the present rates and characteri...
Following a brief overview of the mission concepts for a Mars Global Network Mission as of the time ...
A seismic network on Mars should have enough stations (e.g., 24) to characterize the seismicity of t...
Following a brief overview of the mission concepts for a Mars Global Network Mission as of the time ...
The Final Technical Report on tectonic evolution of Mars is presented. Two papers and an abstract ar...
A three-axis short-period seismometer has been operating on the surface of Mars in the Utopia Planit...
Efforts were made to determine the seismicity of Mars as well as define its internal structure by de...
Seismic experiments on future Mars exploration missions, and the instrumentation required for their ...
By providing a direct view into the interior of the planet, a seismological network on Mars would be...
It is proposed to soft-land three seismometers in the Utopia-Elysium region and three or more radio ...
An objective of future Mars missions involves emplacing a seismic network on Mars to determine the i...
In addition to its intrinsic interest, Mars is particularly well-suited for studying the full range ...
International audienceThe study of the deep interior of Mars suffers from the very limited amount of...
Our fundamental understanding of the interior of the Earth comes from seismology, geodesy, geochemis...
none24siOur fundamental understanding of the interior of the Earth comes from seismology, geodesy, g...
Little is known of the internal structure or composition of Mars or the present rates and characteri...
Following a brief overview of the mission concepts for a Mars Global Network Mission as of the time ...
A seismic network on Mars should have enough stations (e.g., 24) to characterize the seismicity of t...
Following a brief overview of the mission concepts for a Mars Global Network Mission as of the time ...
The Final Technical Report on tectonic evolution of Mars is presented. Two papers and an abstract ar...
A three-axis short-period seismometer has been operating on the surface of Mars in the Utopia Planit...
Efforts were made to determine the seismicity of Mars as well as define its internal structure by de...
Seismic experiments on future Mars exploration missions, and the instrumentation required for their ...
By providing a direct view into the interior of the planet, a seismological network on Mars would be...
It is proposed to soft-land three seismometers in the Utopia-Elysium region and three or more radio ...
An objective of future Mars missions involves emplacing a seismic network on Mars to determine the i...
In addition to its intrinsic interest, Mars is particularly well-suited for studying the full range ...
International audienceThe study of the deep interior of Mars suffers from the very limited amount of...
Our fundamental understanding of the interior of the Earth comes from seismology, geodesy, geochemis...
none24siOur fundamental understanding of the interior of the Earth comes from seismology, geodesy, g...
.svg%3Fwidth%3D300&w=3840&q=75)
Add to ORKG