Habitability, Brine Irradiation and Temperature

Last updated
HABIT
OperatorESA/Roscosmos
ManufacturerOmnisys Instruments AB [1]
Instrument typeTechnology demonstration for IRSU
FunctionHabitability assessment, and harvest atmospheric water on Mars
Mission durationPlanned: ≥ 1 Earth year [2]
Host spacecraft
Spacecraft Kazachok
Operator ESA & Roscosmos
Launch date2028 [3]
Rocket Proton-M/Briz-M
Launch site Baikonur

Habitability, Brine Irradiation and Temperature (HABIT) is an instrument designed to harvest water from the Mars atmosphere, an experiment that might pave the way to future water farms on Mars. [4] As part of ESA's ExoMars-2 mission [2] , the instrument was planned to be placed on board the Kazachok lander. [5] The launch of ExoMars-2 has been postponed to 2028. [3]

Contents

Instrument description

HABIT is composed of two major components: BOTTLE (Brine Observation Transition to Liquid Experiment) and ENVPACK (Environmental Package). BOTTLE contains six containers protected by HEPA filters, filled with salts that will collect atmospheric water through deliquescence. Sensors in each container will measure hydration and a state in which brine formed. Salts in the instrument can be dehydrated to allow indefinite operations of the instrument.[ citation needed ]

ENVPACK will contain instruments measuring ultraviolet irradiance, ground temperature, and a temperature of the atmosphere in three different directions. Most of the ENVPACK instruments were already used in Rover Environmental Monitoring Station of the NASA's Curiosity rover. [6] [ dead link ] The Principal Investigator of HABIT is Javier Martin-Torres. [2]

Scientific objectives

The objectives of HABIT are: [5] [2]

The HABIT instrument will use salts to absorb 5 millilitres of water from the atmosphere each day, and can hold 25 mL in total. If the process works as expected, the technology could be scaled up to provide water for future crewed missions. [4]

Related Research Articles

<i>Phoenix</i> (spacecraft) NASA Mars lander

Phoenix was an uncrewed space probe that landed on the surface of Mars on May 25, 2008, and operated until November 2, 2008. Phoenix was operational on Mars for 157 sols. Its instruments were used to assess the local habitability and to research the history of water on Mars. The mission was part of the Mars Scout Program; its total cost was $420 million, including the cost of launch.

<span class="mw-page-title-main">Life on Mars</span> Scientific assessments on the microbial habitability of Mars

The possibility of life on Mars is a subject of interest in astrobiology due to the planet's proximity and similarities to Earth. To date, no proof of past or present life has been found on Mars. Cumulative evidence suggests that during the ancient Noachian time period, the surface environment of Mars had liquid water and may have been habitable for microorganisms, but habitable conditions do not necessarily indicate life.

<span class="mw-page-title-main">ExoMars</span> Astrobiology programme

ExoMars is an astrobiology programme of the European Space Agency (ESA) and the Russian space agency (Roscosmos).

<span class="mw-page-title-main">Trace Gas Orbiter</span> Mars orbiter, part of ExoMars programme

The ExoMars Trace Gas Orbiter is a collaborative project between the European Space Agency (ESA) and the Russian Roscosmos agency that sent an atmospheric research orbiter and the Schiaparelli demonstration lander to Mars in 2016 as part of the European-led ExoMars programme.

<span class="mw-page-title-main">Martian soil</span> Fine regolith found on the surface of Mars

Martian soil is the fine regolith found on the surface of Mars. Its properties can differ significantly from those of terrestrial soil, including its toxicity due to the presence of perchlorates. The term Martian soil typically refers to the finer fraction of regolith. So far, no samples have been returned to Earth, the goal of a Mars sample-return mission, but the soil has been studied remotely with the use of Mars rovers and Mars orbiters.

<span class="mw-page-title-main">Mars Astrobiology Explorer-Cacher</span> Cancelled NASA Mars rover concept

The Mars Astrobiology Explorer-Cacher (MAX-C), also known as Mars 2018 mission, was a NASA concept for a Mars rover mission, proposed to be launched in 2018 together with the European ExoMars rover. The MAX-C rover concept was cancelled in April 2011 due to budget cuts.

<span class="mw-page-title-main">Seasonal flows on warm Martian slopes</span> Surface features on Mars

Seasonal flows on warm Martian slopes are thought to be salty water flows occurring during the warmest months on Mars, or alternatively, dry grains that "flow" downslope of at least 27 degrees.

Rosalind Franklin, previously known as the ExoMars rover, is a planned robotic Mars rover, part of the international ExoMars programme led by the European Space Agency and the Russian Roscosmos State Corporation. The mission was scheduled to launch in July 2020, but was postponed to 2022. The 2022 Russian invasion of Ukraine has caused an indefinite delay of the programme, as the member states of the ESA voted to suspend the joint mission with Russia; in July 2022, ESA terminated its cooperation on the project with Russia. As of May 2022, the launch of the rover is not expected to occur before 2028 due to the need for a new non-Russian landing platform.

<span class="mw-page-title-main">Rover Environmental Monitoring Station</span>

Rover Environmental Monitoring Station (REMS) is a weather station on Mars for Curiosity rover contributed by Spain and Finland. REMS measures humidity, pressure, temperature, wind speeds, and ultraviolet radiation on Mars. This Spanish project is led by the Spanish Astrobiology Center and includes the Finnish Meteorological Institute as a partner, contributing pressure and humidity sensors.

<i>Schiaparelli</i> EDM Mars landing demonstration system

Schiaparelli EDM was a failed Entry, Descent, and Landing Demonstrator Module (EDM) of the ExoMars programme—a joint mission of the European Space Agency (ESA) and the Russian Space Agency Roscosmos. It was built in Italy and was intended to test technology for future soft landings on the surface of Mars. It also had a limited but focused science payload that would have measured atmospheric electricity on Mars and local meteorological conditions.

<i>Kazachok</i> A planned Mars lander, part of ExoMars programme

The ExoMars Kazachok was a planned robotic Mars lander led by Roscosmos, part of the ExoMars 2022 joint mission with the European Space Agency. Kazachok translates as "Little Cossack", and is also the name of an East Slavic folk dance.

Mars habitability analogue environments on Earth are environments that share potentially relevant astrobiological conditions with Mars. These include sites that are analogues of potential subsurface habitats, and deep subsurface habitats.

The Atmospheric Chemistry Suite (ACS) is a science payload consisting of three infrared spectrometer channels aboard the ExoMars Trace Gas Orbiter (TGO) orbiting Mars since October 2016. The three channels are: the near-infrared channel (NIR), the mid-infrared channel (MIR), and the far infrared channel.

Infrared Spectrometer for ExoMars (ISEM) is an infrared spectrometer for remote sensing that is part of the science payload on board the European Space Agency'sRosalind Franklin rover, tasked to search for biosignatures and biomarkers on Mars. The rover is planned to be launched in August–October 2022 and land on Mars in spring 2023.

ADRON-RM is a neutron spectrometer to search for subsurface water ice and hydrated minerals. This analyser is part of the science payload on board the European Space Agency'sRosalind Franklin rover, tasked to search for biosignatures and biomarkers on Mars. The rover is planned to be launched in August–October 2022 and land on Mars in spring 2023.

WISDOM is a ground-penetrating radar that is part of the science payload on board the European Space Agency'sRosalind Franklin rover, tasked to search for biosignatures and biomarkers on Mars. The rover is planned to be launched in August–October 2022 and land on Mars in spring 2023.

The Fine-Resolution Epithermal Neutron Detector (FREND) is a neutron detector that is part of the instrument payload on board the Trace Gas Orbiter (TGO), launched to Mars in March 2016. This instrument is currently mapping hydrogen levels to a maximum depth of 1 m beneath the Martian surface, thus revealing shallow water ice distribution. This instrument has an improved resolution of 7.5 times over the one Russia contributed to NASA's 2001 Mars Odyssey orbiter.

Nadir and Occultation for MArs Discovery (NOMAD) is a 3-channel spectrometer on board the ExoMars Trace Gas Orbiter (TGO) launched to Mars orbit on 14 March 2016.

Javier Martín-Torres is a Spanish physicist with interests in atmospheric sciences, geophysics, and astrobiology. He has published over 100 scientific papers in these areas.

References

  1. "Omnisys to deliver instrument for the next Mars expedition". Omnisys Instruments. 12 February 2016. Retrieved 13 March 2020.
  2. 1 2 3 4 "ExoMars 2022 surface platform". ESA. 12 March 2020. Retrieved 13 March 2020.
  3. 1 2 "ExoMars: Back on track for the Red Planet".
  4. 1 2 Aron, Jacob (9 December 2015). "Mars moisture-farming mission gets approval for 2018 launch". New Scientist . Retrieved 22 February 2016.
  5. 1 2 "Swedish Mars instrument selected by ESA". Luleå University of Technology . 2 December 2015. Retrieved 5 December 2015.
  6. "Instrument – Atmospheric Science Group". Luleå University of Technology . Retrieved 22 February 2016.