Mission type | Enceladus Orbiter and Lander |
---|---|
Operator | NASA |
Website | https://space.jhuapl.edu/projects-and-studies/enceladus-orbilander |
Mission duration |
|
Spacecraft properties | |
Manufacturer | APL (proposed) |
Launch mass | 6610 kg [1] : 18 |
Dry mass | 2690 kg |
Power | 741 W (at launch) 589 W (landing) |
Start of mission | |
Launch date | October 2038 (proposed) [1] : 33 |
Rocket | Space Launch System Block 2 (proposed) |
Launch site | Kennedy Space Center, Pad 39B |
Contractor | NASA |
Flyby of Jupiter | |
Closest approach | October 2040 (proposed) |
Distance | 4,730,000 km (2,940,000 mi) |
Saturn orbiter | |
Orbital insertion | August 2045 (proposed) |
Orbital departure | early 2050 (proposed) |
Enceladus orbiter | |
Orbital insertion | early 2050 (proposed) |
Orbital departure | mid 2051 (proposed) |
Enceladus lander | |
Landing date | mid 2051 (proposed) |
Large Strategic Science Missions Planetary Science Division |
The Enceladus Orbilander is a proposed NASA Flagship mission to Saturn's moon Enceladus. The Enceladus Orbilander would spend a year and a half orbiting Enceladus and sampling its water plumes,which stretch into space,before landing on the surface for a two-year mission to study materials for evidence of life. [1] The mission,with an estimated cost of $4.9 billion,could launch in the late 2030s on a Space Launch System or Falcon Heavy with a landing in the early 2050s. It was proposed in the 2023–2032 Planetary Science Decadal Survey as the third highest priority Flagship mission,after the Uranus Orbiter and Probe and the Mars Sample Return program. [2]
At 500 kilometres (310 miles) in diameter,Enceladus is the sixth largest moon of Saturn and the 19th largest in the solar system. [3] Enceladus has been visited and imaged in detail by three other probes:the twin Voyager spacecraft,and the Saturn orbiting Cassini spacecraft. Out of these,Cassini investigated Enceladus in the most detail and contributed the most to the current scientific understanding of Enceladus. Cassini's 23 targeted close flybys [4] helped discover that Enceladus is a geologically active world,with young (recently formed/solidified) terrain. The flybys also showed active,warm water plumes,along with evidence hinting at a subsurface ocean. [5] Cassini also provided evidence of hydrothermal processes driving both the geysers and Enceladus' active geology,making the moon one of the most attractive places to find life within the solar system.
After Cassini's mission,a variety of proposals to follow-up on Cassini's findings at Enceladus. [6] Journey to Enceladus and Titan,an astrobiology mission to Enceladus and Titan,competed for the 13th Discovery Program mission but was not selected. [7] [8] Later,In 2017,two Enceladus focused astrobiology missions,Enceladus Life Signatures and Habitability and Enceladus Life Finder competed for the 4th New Frontiers mission,but were ultimately not selected. [9] [10]
The Enceladus Orbilander proposal was created by a team led by Shannon MacKenzie to support the Planetary Science Decadal Survey. [11] While previous mission studies had investigated multiple flybys to study Enceladus,MacKenzie's team,studying a Flagship mission architecture with a greater budget cap,decided to study an orbiter,lander,or a combination thereof. [12] Ultimately,the decision to combine the orbiter and lander into one spacecraft was informed by Enceladus' small size and negligible gravity,which results in trivial delta-v to land. [13] In the 2022-2032 Planetary Decadal Survey,the Enceladus Orbilander was recommended as the third highest priority new flagship mission. [14] The selection was motivated by proposal's exobiology and planetary habitability focus. [15]
Due to Enceladus's small size,the amount of energy required to land compared to capturing into orbit is negligible. Therefore,the Enceladus Orbilander is envisioned uniquely combine both the functions of an orbiter and a lander into a single spacecraft. [16]
The proposed spacecraft will carry three separate instrument suites and a sampling system. Each instrument suite is tailored towards a different regime of science operations.
The proposed instruments are: [1] : 10,B7-B10
Instrument | Heritage Instrument (Mission) | Science Suite |
---|---|---|
High-Resolution Mass Spectrometer (HRMS) | MASPEX (Europa Clipper) | Life Detection Suite |
Separation Mass Spectrometer (SMS) | Sample Analysis at Mars (Curiosity) | |
Electrochemical Sensor Array (ESA) | Wet Chemistry Laboratory (Phoenix) | |
Microcapillary Electrophoresis-Laser Induced Fluorescence | N/A | |
Microscope | MECA Atomic Force Microscope (Phoenix) | |
Solid State Nanopore Sequencer | N/A | |
Narrow Angle Camera (NAC) | Long Range Reconnaissance Imager ( New Horizons ) | Life Detection Suite |
Wide Angle Camera (WAC) | ECAM-M50 (Janus) | |
Thermal Emission Spectrometer (TES) | Mercury Radiometer and Thermal Infrared Spectrometer (BepiColombo) | |
Context Imager | Stereo Surface Imager (Phoenix) | In Situ Suite |
Seismometer | Seismic Experiment for Interior Structure (Insight) | |
Additionally,three separate sampling systems are proposed for each stage of flight:a 1 square meter funnel to passively collect particles,a scoop for active particle collection on the surface,and a gas inlet for gas emissions. [1] : 10,B11
The Enceladus Orbilander is proposed to be launched in October 2038. [1] : 4 The spacecraft is proposed to be launched by a Space Launch System Block II variant with a Castor 30B upper stage,although a Falcon Heavy has also been considered but would require the spacecraft to launch on a slower trajectory with flybys of Venus. [1] : 7 The spacecraft's proposed launch is timed so that a Jupiter gravity assist can be performed in October 2040 to save propellant for Saturn orbital insertion in August 2045. [1] : 19 In Saturn orbit,the spacecraft will embark on a complex,4.5 year long tour of the moons of Saturn,using gravity assists off moons such as Titan,Rhea,Dione,and Tethys to lower the orbital inclination of the spacecraft. [1] : 21-22 After a series of flybys with Enceladus itself,the spacecraft will enter Enceladus orbit.
The spacecraft will spend 1.5 years in a 12 hours long elliptical orbit around Enceladus. [1] : 20 The closest point of the orbit to the surface will pass over the south polar tiger stripes to collect plume particles and remote sensing data. Whilst orbiting Enceladus,mission planners will use high resolution images and other data to determine a safe landing ellipse. [13] When mission planners decide to land the spacecraft,the Enceladus Orbilander will lower its orbit and begin a powered descent towards the surface. The spacecraft will use terrain-relative navigation similar to systems used on OSIRIS-REx to avoid hazards during the descent. [16] When the spacecraft is 10 metres (33 ft) above the surface,the main engine shuts off to avoid contaminating the area,and the spacecraft pitches to its side before soft landing. [1] : 16
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.
Enceladus is the sixth-largest moon of Saturn and the 18th-largest in the Solar System. It is about 500 kilometers in diameter, about a tenth of that of Saturn's largest moon, Titan. It 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 reaches only −198 °C, far colder than a light-absorbing body would be. Despite its small size, Enceladus has a wide variety of surface features, ranging from old, heavily cratered regions to young, tectonically deformed terrain.
This article provides a timeline of the Cassini–Huygens mission. Cassini was a collaboration between the United States' NASA, the European Space Agency ("ESA"), and the Italian Space Agency ("ASI") to send a probe to study the Saturnian system, including the planet, its rings, and its natural satellites. The Flagship-class uncrewed robotic spacecraft comprised both NASA's Cassini probe, and ESA's Huygens lander which was designed to land on Saturn's largest moon, Titan. Cassini was the fourth space probe to visit Saturn and the first to enter its orbit. The craft were named after astronomers Giovanni Cassini and Christiaan Huygens.
The New Frontiers program is a series of space exploration missions being conducted by NASA with the purpose of furthering the understanding of the Solar System. The program selects medium-class missions which can provide high science returns.
The exploration of Saturn has been solely performed by crewless probes. Three missions were flybys, which formed an extended foundation of knowledge about the system. The Cassini–Huygens spacecraft, launched in 1997, was in orbit from 2004 to 2017.
Titan Saturn System Mission (TSSM) was a joint NASA–ESA proposal for an exploration of Saturn and its moons Titan and Enceladus, where many complex phenomena were revealed by Cassini. TSSM was proposed to launch in 2020, get gravity assists from Earth and Venus, and arrive at the Saturn system in 2029. The 4-year prime mission would include a two-year Saturn tour, a 2-month Titan aero-sampling phase, and a 20-month Titan orbit phase.
Titan Mare Explorer (TiME) is a proposed design for a lander for Saturn's moon Titan. TiME is a relatively low-cost, outer-planet mission designed to measure the organic constituents on Titan and would have performed the first nautical exploration of an extraterrestrial sea, analyze its nature and, possibly, observe its shoreline. As a Discovery-class mission it was designed to be cost-capped at US$425 million, not counting launch vehicle funding. It was proposed to NASA in 2009 by Proxemy Research as a scout-like pioneering mission, originally as part of NASA's Discovery Program. The TiME mission design reached the finalist stage during that Discovery mission selection, but was not selected, and despite attempts in the U.S. Senate failed to get earmark funding in 2013. A related Titan Submarine has also been proposed.
The Planetary Science Decadal Survey is a serial publication of the United States National Research Council produced for NASA and other United States Government Agencies such as the National Science Foundation. The documents identify key questions facing planetary science and outlines recommendations for space and ground-based exploration ten years into the future. Missions to gather data to answer these big questions are described and prioritized, where appropriate. Similar decadal surveys cover astronomy and astrophysics, earth science, and heliophysics.
The Uranus Orbiter and Probe is an orbiter mission concept to study Uranus and its moons. The orbiter would also deploy an atmospheric probe to characterize Uranus's atmosphere. The concept is being developed as a potential large strategic science mission for NASA. The science phase would last 4.5 years and include multiple flybys of each of the major moons.
The Cassini space probe was deliberately disposed of via a controlled fall into Saturn's atmosphere on September 15, 2017, ending its nearly two-decade-long mission. This method was chosen to prevent biological contamination of any of the moons of Saturn now thought to offer potentially habitable environments. Factors that influenced the mission end method included the amount of rocket fuel left, the health of the spacecraft, and funding for operations on Earth.
Enceladus Life Finder (ELF) is a proposed astrobiology mission concept for a NASA spacecraft intended to assess the habitability of the internal aquatic ocean of Enceladus, which is Saturn's sixth-largest moon of at least 146 total moons, and seemingly similar in chemical makeup to comets. The spaceprobe would orbit Saturn and fly through Enceladus's geyser-like plumes multiple times. It would be powered by energy supplied from solar panels on the spacecraft.
Journey to Enceladus and Titan (JET) is an astrobiology mission concept to assess the habitability potential of Enceladus and Titan, moons of Saturn.
Life Investigation For Enceladus (LIFE) was a proposed astrobiology mission concept that would capture icy particles from Saturn's moon Enceladus and return them to Earth, where they could be studied in detail for signs of life such as biomolecules.
THEO is a feasibility study for a New Frontiers class orbiter mission to Enceladus that would directly sample its south pole water plumes in order to study its internal habitability and to search for biosignatures. Specifically, it would take advantage of the direct sampling opportunities of a subsurface ocean.
Oceanus is a NASA/JPL orbiter mission concept proposed in 2017 for the New Frontiers mission #4, but it was not selected for development. If selected at some future opportunity, Oceanus would travel to Saturn's moon Titan to assess its habitability. Studying Titan would help understand the early Earth and exoplanets which orbit other stars. The mission is named after Oceanus, the Greek god of oceans.
Explorer of Enceladus and Titan (E2T) is a space mission concept that would investigate the evolution and habitability of the Saturnian satellites Enceladus and Titan and is proposed by the European Space Agency in collaboration with NASA.
Enceladus Life Signatures and Habitability (ELSAH) is an astrobiology concept mission proposed in 2017 to NASA's New Frontiers program to send a spacecraft to Enceladus to search for biosignatures and assess its habitability. The Principal Investigator is Christopher P. McKay, an astrobiologist at NASA Ames Research Center, and the managing NASA center is Goddard Space Flight Center. No details of the mission have been made public, but observers speculate that it would be a plume-sampling orbiter mission.
The Ocean Worlds Exploration Program (OWEP) is a NASA program to explore ocean worlds in the outer Solar System that could possess subsurface oceans to assess their habitability and to seek biosignatures of simple extraterrestrial life.
Christopher R. Glein is an American geochemist at the Southwest Research Institute in San Antonio, TX. He studies planetary science, astrobiology, and organic geochemistry. Glein was the first to describe how Saturn's moon Enceladus is the only known body, besides Earth, that has all of the requirements necessary for life. Glein has been involved in multiple spacecraft missions, leading to significant findings about Pluto, Enceladus, and Titan. In 2017, he was recognized for Outstanding Contributions to the ESA Rosetta Mission by the European Space Agency.
Neptune Odyssey is an orbiter mission concept to study Neptune and its moons, particularly Triton. The orbiter would enter into a retrograde orbit of Neptune to facilitate simultaneous study of Triton and would launch an atmospheric probe to characterize Neptune's atmosphere. The concept is being developed as a potential large strategic science mission for NASA by a team led by the Applied Physics Laboratory at Johns Hopkins University. The current proposal targets a launch in 2033 using the Space Launch System with arrival at Neptune in 2049, although trajectories using gravity assists at Jupiter have also been considered with launch dates in 2031.
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