Seismic Experiment for Interior Structure
Testing of the lander's robotic arm that will deploy the seismometer
|Instrument type||geophysical observations|
|Mission duration||Planned: 2 years on Mars Current: 20 sols (20 days) since landing|
|Began operations||Landing: 26 November 2018|
|Mass||29.5 kg (65 lb)|
|Dimensions||Vacuum chamber volume: 3 L (0.66 imp gal; 0.79 US gal)|
|Power consumption||8.5 W|
|Data rate||38 megabits/day |
|Launch date||5 May 2018, 11:05UTC|
The Seismic Experiment for Interior Structure (SEIS) is a seismometer and the primary scientific instrument on board the InSight Mars lander launched on 5 May 2018 for a landing on 26 November 2018. SEIS is expected to provide seismic measurements of Mars, enabling researchers to develop 3D structure maps of the deep interior. By better understanding the Martian interior, it will trigger a better understanding of the Earth, Moon, and rocky planetary bodies in general.
As of 26 November 2018, SEIS is still inside the InSight lander. The mission will take up to three months to deploy and commission the geophysical science instruments. It will then begin its mission of observing Mars, which is planned to last for two years.
Mars is the fourth planet from the Sun; it is about 1/2 size of Earth with 1/3 the gravity, and orbits between about 1.3 to 1.7 Earth-Sun distances. It has an almost 25-hour day, and has a 2-year orbit of the Sun for its year. Flybys and landings to gather scientific data about Mars have been conducted since the 1960s, but quality seismological studies – which would provide detailed information about the interior of Mars – have yet to be performed.
Only two astronomical bodies – the Earth and the Moon – have been studied in this way, and learning about Mars is hoped to have a ripple effect on understanding the geology of all rocky planetary bodies. Other onboard instruments working in synergy with SEIS are the Temperature and Winds for InSight module, the Heat Flow and Physical Properties Package, and the Rotation and Interior Structure Experiment.
While two seismometers were landed on Mars during the Viking missions in 1976, results were limited. Seismometers on both Viking spacecraft were mounted on the lander, which meant that it also picked up vibrations from various operations of the lander and caused by the wind. In addition, the Viking 1 lander's seismometer did not deploy properly.
The seismometer readings were used to estimate a Martian geological crust thickness between 14 and 18 km (8.7 and 11.2 mi) at the Viking 2 lander site. Unexpectedly, the seismometer also detected pressure from the Mars winds, complementing the meteorology results. A single possible candidate for a marsquake was recorded, although it was not confirmed due to the limitations of the design, and interference from other sources of vibration such as wind. Despite these limitations, it was clear that widespread and large marsquakes were not detected.
SEIS is the primary instrument of the InSight mission, and it was designed and produced by the French Space Agency (CNES), with the participation of the Institut de Physique du Globe de Paris (IPGP), the Swiss Federal Institute of Technology (ETH), the Max Planck Institute for Solar System Research (MPS), Imperial College, Institut supérieur de l'aéronautique et de l'espace (ISAE) and JPL. The Principal Investigator is Philippe Lognonné from the Institute of Earth Physics of Paris (Institut de Physique du Globe de Paris), in the E.U.
Its design consists of a 3-axis very-broad-band seismometer (enclosed in a vacuum thermal enclosure) and a 3-axis short-period instrument. Mars is expected to have lower seismic activity than Earth, so minimisation of wind vibrations is critical. The whole assembly is placed under a heavy wind and thermal shield designed to minimize thermal contrasts and offer some protection against gusts of wind.
The tripod-mounted seismometer will take precise measurements of marsquakes and other internal activity on Mars to better understand the planet's history and internal structure. It will also investigate how the Martian crust and mantle respond to the effects of meteorite impacts, which gives clues to the planet's inner structure. The seismometer will also detect sources including atmospheric waves and gravimetric signals (tidal forces) from Mars' moon Phobos, up to high-frequency seismic waves at 50 Hz.
The SEIS instrument is deployed by the Instrument Deployment System, a robotic arm that can position the sensor directly on the surface. The instrument is supported by a suite of meteorological sensors (TWINS) to characterize atmospheric disturbances that might affect the measurements. These include a vector magnetometer provided by UCLA that will measure magnetic disturbances such as those caused by the Martian ionosphere; a suite of air temperature, wind speed and wind direction sensors based on the Spanish/Finnish Rover Environmental Monitoring Station; and a barometer from JPL.
During the final integration of SEIS, several small leaks were found in the vacuum thermal enclosure. This forced the postponement of the InSight launch from 2016 to 2018, and the redesign of a new enclosure under the supervision of JPL. The cost of the delay was estimated to be US$150 million.
Routine operations will be split into two services, the Mars Structure Service (MSS) and Marsquake Service (MQS), which will be responsible, respectively, for defining the structure models and seismic activity. Combination of data with results from the InSight radio science and orbital observations will allow for constraint of the deeper structure.
Possible observations include:
- P waves and S waves
- Meteor strikes (see also Category:Meteorites found on Mars)
- Tidal forces from Mars' moons
- Interior revelations, such as the presence of a solid or liquid core and its size
During development, the power of multiple sites was noted, but one site offers a tremendous insight to the interior. With a single site, the location of a marsquake event can be constrained to the surface of a sphere, by measuring what are known as P-waves and S-waves.
There is a variety of single-site seismology techniques that can yield data, for example, the detection of an impact on the surface by a meteorite for which the location is identified. If Mars has large marsquakes, they may allow the deep interior to be determined. As the vibrations pass through the planet they are affected by the properties of the materials and its configuration.
For example, the effect of tidal forces on Mars by Phobos, which should be about 10 mm, would be noticeably affected by a liquid Mars core. Even without any marsquake, it should be possible after about six months of observation to use this method to increase or decrease the likelihood Mars has a liquid core.
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