Mars atmospheric entry


Mars atmospheric entry is the entry into the atmosphere of Mars. High velocity entry into Martian air creates a CO2-N2 plasma, as opposed to O2-N2 for Earth air. Mars entry is affected by the radiative effects of hot CO2 gas and Martian dust suspended in the air. Flight regimes for entry, descent, and landing systems include aerocapture, hypersonic, supersonic, and subsonic.

Overview

Thermal protection systems and atmospheric friction have been used historically to reduce most of the kinetic energy that needs to be lost prior to landing, with parachutes and, sometimes, a final bit of retropropulsion used in the final landing. High-altitude high-velocity retropropulsion is being researched for future transport flights landing heavier cargos.
For example, Mars Pathfinder entered in 1997. About 30 minutes prior to entry, the cruise stage and entry capsule separated. When the capsule hit the atmosphere it decelerated from about 7.3 km/s to 0.4 km/s over three minutes. As it descended the parachute opened to slow it down further, and soon after the heat shield was released. During entry a signal was relayed back to Earth, including semaphore signals for important events.

List of spacecraft

Technologies

A deployable decelerator like a parachute can slow down a spacecraft after a heat shield. Typically a Disk-Gap-Band parachute has been used, but another possibility are trailing or attached inflatable entry devices. Inflatable types include sphere w/ fence, teardrop w/ fence, isotensoid, torus, or tension cone and attached types include isotensoid, tension cone, and stacked toroid blunted cone. Viking Program era researchers were the true pioneers of this technology, and development had to be restarted after decades of neglect. Those latest studies have shown that tension cone, isotensoid, and stacked torus may be the best types to pursue.
Finland's MetNet probe may use an expandable entry shield if it is sent. Martian air can also be used for aerobraking to orbital velocity, rather than descent and landing. Supersonic retro-propulsion is another concept to shed velocity.
NASA is carrying out research on retropropulsive deceleration technologies to develop new approaches to Mars atmospheric entry. A key problem with propulsive techniques is handling the fluid flow problems and attitude control of the descent vehicle during the supersonic retropropulsion phase of the entry and deceleration. More specifically, NASA is carrying out thermal imaging infrared sensor data-gathering studies of the SpaceX booster controlled-descent tests that are currently,, underway.
The research team is particularly interested in the altitude range of the SpaceX "reentry burn" on the Falcon 9 Earth-entry tests as this is the "powered flight through the Mars-relevant retropulsion regime" that models Mars entry and descent conditions, although SpaceX is of course interested also in the final engine burn and lower velocity retropropulsive landing as well since that is a critical technology for their reusable booster development program which they hope to use for Mars landings in the 2020s.

Examples

Mars Science Laboratory

The following data were compiled for the Mars Science Laboratory by the Entry, Descent and Landing team at the NASA's Jet Propulsion Laboratory. It provides a timeline of critical mission events that occurred on the evening of August 5 PDT.
EventTime of Event Occurrence at Mars Time Event Occurrence Received on Earth
Atmospheric entry10:10:45.7 PM10:24:33.8 PM
Parachute deployment10:15:04.9 PM10:28:53.0 PM
Heat shield separation10:15:24.6 PM10:29:12.7 PM
Rover lowered by the sky crane10:17:38.6 PM10:31:26.7 PM
Touchdown10:17:57.3 PM10:31:45.4 PM

Curiosity's EDL team releases a timeline for mission milestones surrounding the landing of the Mars rover.

Landing site identification

Concept art of a Mars lander as it approaches the surface, illustrating how identifying a safe landing spot is a concern.