This illustration of the InSight lander on Mars shows the location of its science instruments, including a drill to explore below the surface.
Artist's Concept of InSight Lander on Mars: InSight was the first mission dedicated to investigating the deep interior of Mars. The findings advance understanding of how all rocky planets, including Earth, formed and evolved.
NASA/JPL-Caltech

Seismic Experiment for Interior Structure (SEIS)

A robotic arm hovers above a small dome structure on the flat red surface of Mars.
This image shows InSight's domed Wind and Thermal Shield, which covers its seismometer.
NASA/JPL-Caltech

InSight’s seismometer, SEIS, the Seismic Experiment for Interior Structure, was a round, dome-shaped instrument that sat on the Martian surface and took the "pulse" or seismic vibrations of Mars. Its measurements provided a glimpse into the planet’s internal activity. The seismometer waited patiently to sense the pulse, or seismic waves, from marsquakes, and thumps of meteorite impacts. A suite of wind, pressure, temperature, and magnetic field sensors helped fine-tune the seismometer's measurements. This helped it sense surface vibrations generated by weather systems such as dust storms, or by turbulence in the atmosphere due to phenomena such as dust devils, which can also generate seismic waves. SEIS measurements told scientists about the nature of the material that first formed the rocky planets of the solar system.

Tech Specs

Main Job
To measure the pulse of Mars by studying waves created by marsquakes, thumps of meteorite impacts, and even surface vibrations generated by activity in Mars' atmosphere and by weather phenomena such as dust storms.
Location
Placed on the surface of Mars
Power
Up to 8.5 watts
Volume
About 0.8 gallons (3 liters)
Data Return
38 megabits per day

Heat Flow and Physical Properties Package (HP3)

Two pieces of cylindrical science equipment are stacked on the flat red surface of Mars.
NASA's InSight lander set its heat probe, called the Heat and Physical Properties Package (HP3)
NASA/JPL-Caltech

The Heat Flow and Physical Properties Package, HP3 for short, was designed to burrow down to almost 16 feet (5 meters) into Mars' surface. That's deeper than any previous arms, scoops, drills, or probes before it. Similar to studying the heat leaving a car engine, it sought to measure the heat coming from Mars' interior to reveal how much heat was flowing out of the body of the planet, and what the source of the heat was. This instrument was designed to help scientists determine whether Mars formed from the same stuff as Earth and the Moon, and to give them a sneak peek into how the planet evolved.

The HP3 was designed, built and managed by the German Aerospace Center (Deutsches Zentrum für Luft- und Raumfahrt, or DLR), with significant contributions from the Space Research Center (CBK) of the Polish Academy of Sciences and Astronika.

Tech Specs

Main Job
HP3 was designed to measure the heat flowing out of the interior of the planet, allowing us to infer Mars' temperature deep in the planet.
Location
Mounted on the lander deck for the trip to Mars. After landing, the lander's arm picked up HP3 and placed it on the surface. The mole then began to hammer itself under the surface but encountered different soil properties than expected and was unable to reach the desired depth.
Mass
Just over 6.5 pounds (about 3 kilograms), including the control electronics inside the lander.
Power
A maximum of 2 watts while burrowing underneath the surface.
Volume
About 5.3 gallons (20 liters) in total, including the control electronics inside the lander.
Data Return
350 megabits over the course of the mission

Rotation and Interior Structure Experiment (RISE)

An artist's concept of InSight on Mars with location of the two antennas on either side of its science instrument deck.
Artist's Concept of InSight Lander on Mars: InSight was the first mission dedicated to investigating the deep interior of Mars. The findings will advance understanding of how all rocky planets, including Earth, formed and evolved.
NASA/JPL-Caltech

InSight’s Rotation and Interior Structure Experiment, RISE, precisely tracked the location of the lander to determine just how much Mars' north pole wobbles as it orbits the Sun. These observations provide detailed information on the size, composition, and characteristics of Mars' iron-rich core.

Tech Specs

Main Job
RISE tracked the wobble of Mars' north pole as the Sun pushes and pulls it in its orbit. This helps scientists determine the size and composition of Mars' core.
Location
Mounted on the lander deck for the trip to Mars. After landing, the lander's arm picked up HP3 and placed it on the surface. The mole then began to hammer itself under the surface but encountered different soil properties than expected and was unable to reach the desired depth.
Mass
About 16 pounds (7.3 kilograms).
Antennas
3 pounds (1.4 kilograms).
Transponder and Transmitter
9.6 pounds (4.4 kilograms).
Power
78 Watts (operated up to one hour per day).
Volume
0.7 cubic feet (19.8 liters) total.
Electronics
0.13 cubic feet (3.8 liters).
Medium Gain Antennas
0.57 cubic feet (16 liters).
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