Journey to Enceladus and Titan

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Journey to Enceladus and Titan (JET) is an astrobiology mission concept to assess the habitability potential of Enceladus and Titan, moons of Saturn.

Contents

The JET orbiter concept was proposed in 2011 by the Jet Propulsion Laboratory to NASA's Discovery Program for its 13th mission, but it was not selected as a semi-finalist; Lucy was selected on January 4, 2017. [1] [2]

Concept

Enceladus full view Enceladus - July 15 2005 (36690644854).jpg
Enceladus full view

Enceladus is a small icy moon, seemingly similar in chemical makeup to comets, [3] with jets or geysers of water erupting from its surface that might be connected to active hydrothermal vents at its subsurface water ocean floor, [4] [5] [6] [7] [8] where the moon's ocean meets the underlying rock, a prime habitat for life. [9] [10] The geysers could provide easy access for sampling the moon's subsurface ocean, and if there is microbial life in it, ice particles from the sea could contain the evidence astrobiologists need to identify them. [11] An organic-rich world, Titan has a methane cycle comparable in atmospheric and geological processes to Earth's water cycle.

Enceladus's south pole - Geysers spray water from many locations along the 'tiger stripes' feature. Enceladus geysers June 2009.jpg
Enceladus's south pole - Geysers spray water from many locations along the 'tiger stripes' feature.

The JET orbiter mission concept was proposed in 2011 by the Jet Propulsion Laboratory to NASA's Discovery Program Mission #13. [12] During the orbiter's one-year mission, it would perform high-resolution mass spectroscopy mapping that would determine what processes have shaped and are shaping the moons, and it would permit assessment of the habitability potential of Enceladus and Titan. [8] [12]

In order to meet the $450 million cost cap, the orbiter would carry only two instruments. It would orbit Saturn and make a total of 16 flybys of Enceladus and Titan, the closest ones at 900 km from Titan's surface. [12] In June 2015 NASA announced a list of five finalists for the current competition, but the Journey to Enceladus and Titan proposal was not selected. Lucy was selected on January 4, 2017, and is planned to launch in October 2021. [1] [2]

Objectives

Titan's mystery clouds PIA21054 - Titan's Mystery Clouds.jpg
Titan's mystery clouds
Near-infrared radiation from the Sun reflecting off Titan's hydrocarbon seas. Specular Spectacular (PIA18432).jpg
Near-infrared radiation from the Sun reflecting off Titan's hydrocarbon seas.

The three goals of the mission are to determine the processes that have shaped and are shaping Enceladus and Titan, to assess their astrobiological potential, and to investigate their formation and evolution. [12] [13]

At Enceladus, the mission will determine composition and flux of material in the plume, and will produce temperature maps of the faults, tectonics and interior dynamics. [13] At Titan, it will characterize of the organic molecules in the upper atmosphere at different altitudes (> 900 km) and latitudes, and will produce high-resolution images for detailed study of features forming at different time-scales. [13]

Launch and trajectory

If using an Atlas V rocket, JET would reach Saturn in 8.5 years using a Venus–Earth–Earth gravity assist trajectory. [13]

Payload

The orbiter payload consists of two instruments: [12] [13]

See also

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Astrobiology is a scientific field within the life and environmental sciences that studies the origins, early evolution, distribution, and future of life in the universe by investigating its deterministic conditions and contingent events. As a discipline, astrobiology is founded on the premise that life may exist beyond Earth.

<span class="mw-page-title-main">Saturn</span> Sixth planet from the Sun

Saturn is the sixth planet from the Sun and the second-largest in the Solar System, after Jupiter. It is a gas giant with an average radius of about nine and a half times that of Earth. It has only one-eighth the average density of Earth, but is over 95 times more massive.

<span class="mw-page-title-main">Titan (moon)</span> Largest moon of Saturn

Titan is the largest moon of Saturn, the second-largest in the Solar System and larger than any of the dwarf planets of the Solar System. It is the only moon known to have a dense atmosphere, and is the only known object in space other than Earth on which clear evidence of stable bodies of surface liquid has been found.

<i>Cassini–Huygens</i> Space research mission sent to the Saturnian system

Cassini–Huygens, commonly called Cassini, was a space-research mission by NASA, the European Space Agency (ESA), and the Italian Space Agency (ASI) to send a space probe to study the planet Saturn and its system, including its rings and natural satellites. The Flagship-class robotic spacecraft comprised both NASA's Cassini space probe and ESA's Huygens lander, which landed on Saturn's largest moon, Titan. Cassini was the fourth space probe to visit Saturn and the first to enter its orbit, where it stayed from 2004 to 2017. The two craft took their names from the astronomers Giovanni Cassini and Christiaan Huygens.

<span class="mw-page-title-main">Iapetus (moon)</span> Moon of Saturn

Iapetus is a moon of Saturn. It is the 24th of Saturn’s 83 known moons. With an estimated diameter of 1,469 km, it is the third-largest moon of Saturn and the eleventh-largest in the Solar System. Named after the Titan Iapetus, the moon was discovered in 1671 by Giovanni Domenico Cassini.

<span class="mw-page-title-main">Enceladus</span> Natural satellite orbiting Saturn

Enceladus is the sixth-largest moon of Saturn. It is about 500 kilometers in diameter, about a tenth of that of Saturn's largest moon, Titan. Enceladus is mostly covered by fresh, clean ice, making it one of the most reflective bodies of the Solar System. Consequently, its surface temperature at noon only reaches −198 °C, far colder than a light-absorbing body would be. Despite its small size, Enceladus has a wide range of surface features, ranging from old, heavily cratered regions to young, tectonically deformed terrain.

Timeline of <i>Cassini–Huygens</i> Timeline of notable events in the history of the Cassini–Huygens mission

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<span class="mw-page-title-main">Tiger stripes (Enceladus)</span>

The tiger stripes of Enceladus consist of four sub-parallel, linear depressions in the south polar region of the Saturnian moon. First observed on May 20, 2005 by the Cassini spacecraft's Imaging Science Sub-system (ISS) camera, the features are most notable in lower resolution images by their brightness contrast from the surrounding terrain. Higher resolution observations were obtained by Cassini's various instruments during a close flyby of Enceladus on July 14, 2005. These observations revealed the tiger stripes to be low ridges with a central fracture. Observations from the Composite Infrared Spectrometer (CIRS) instrument showed the tiger stripes to have elevated surface temperatures, indicative of present-day cryovolcanism on Enceladus centered on the tiger stripes.

<span class="mw-page-title-main">Exploration of Saturn</span> Overview of the exploration of Saturn

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<i>Cassini</i> retirement Retirement of NASAs Cassini spacecraft on 15 September 2017

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<span class="mw-page-title-main">Enceladus Life Finder</span> Proposed NASA mission to a moon of Saturn

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Enceladus Explorer (EnEx) is a planned interplanetary orbiter and lander mission equipped with a subsurface maneuverable ice melting probe suitable to assess the existence of life on Saturn's moon Enceladus.

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<span class="mw-page-title-main">Oceanus (Titan orbiter)</span>

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References

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