Uranus Orbiter and Probe

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Voyager 2 is the only space probe to have visited the Uranus system, completing a flyby on January 24, 1986. The 2011-2022 Planetary Science Decadal Survey recommended a Flagship-class orbiter mission to an ice giant with priority behind what would become the Mars 2020 rover and the Europa Clipper. [5] [6] [7] Ice giants are now appreciated as a common type of exoplanet, precipitating the need for further study of ice giants in the Solar System. [8] The ice giants Uranus and Neptune were seen as unique yet equally compelling scientific targets, but a Uranus orbiter and atmospheric probe was given preference for logistical and cost reasons. [5] [7] A Uranus orbiter would logically follow Flagship-class orbiter missions undertaken at Jupiter and Saturn ( Galileo and Cassini , respectively).

In 2017, prior to the 2023–2032 survey, a committee narrowed twenty mission concepts to three scenarios for Uranus and a fourth for Neptune. [8] [9] [10] [11] A mission to Neptune is viewed by some to be of greater scientific merit [12] because Triton, likely a captured Kuiper belt object and ocean world, is a more compelling astrobiology target than the moons of Uranus (though Ariel and Miranda in particular are possible ocean worlds). [13] There was also a study that considered a New Frontiers-level Uranus orbiter mission concept if a Flagship-class mission to Neptune were favored. [14] Nevertheless, again due to cost and logistical considerations including launch vehicle availability and available launch windows, the 2023–2032 Planetary Science Decadal Survey recommended the Uranus Orbiter and Probe instead of an analogous proposal for Neptune, Neptune Odyssey. [3] [4]

Key science questions

The orbiter paired with an atmospheric probe will address a variety of scientific questions across all aspects of the Uranus system: [3]

Origin, interior, and atmosphere

Magnetosphere

Satellites and rings

  • What are the internal structures and rock-to-ice ratios of the large Uranian moons and which moons possess substantial internal heat sources or possible oceans?
  • How do the compositions and properties of the Uranian moons constrain their formation and evolution?
  • What geological history and processes do the surfaces record and how can they inform outer solar system impactor populations? What evidence of exogenic interactions do the surfaces display?
  • What are the compositions, origins and history of the Uranian rings and inner small moons, and what processes sculpted them into their current configuration?

Mission details

Schematic of the 2021 concept study design for the Orbiter and Probe 2021 Uranus Orbiter and Probe schematic.jpg
Schematic of the 2021 concept study design for the Orbiter and Probe

The atmospheric probe element of this mission would study the vertical distribution of cloud-forming molecules, thermal stratification, and wind speed as a function of depth. The 2010 mission design envisioned a probe of 127 kg (280 lb), less than half that of the Galileo atmospheric probe. [7] A later design study suggested results could be significantly enhanced by adding a second probe which could be as small as 30 kg (66 lb) in mass and about 0.5 m (20 in) in diameter. [15]

Orbiter instruments

The orbiter is proposed to carry the following instruments in the baseline concept, with additional instruments possible should they prove to be within mass, power, and cost limitations: [1]

Uranus Orbiter and Probe
Uranus Montage.jpg
Mosaic of images of Uranus and its 5 major moons from Voyager 2
Mission type Uranus orbiter
Operator NASA
Mission durationCruise: 13.4 years
Science phase: 4.5 years [1]
Spacecraft properties
Launch mass7,235 kg (15,950 lb) [1]
Dry mass2,756 kg (6,076 lb) [1]
Payload mass60.5 kg (133 lb) plus 19.7 kg (43 lb) atmospheric probe [1]
DimensionsHeight: 7.1 m (23 ft)
Diameter: less than 5 m (16 ft) [1]
Power735 W (0.986 hp) from 3 Mod1 Next-Generation Radioisotope thermoelectric generators [1]
Start of mission
Launch datenot earlier than 2031 [1] [2]
Rocket Falcon Heavy Expendable (proposed) [1]
Launch site Kennedy Space Center Launch Complex 39A (proposed) [1]
Flyby of Earth (gravity assist)
Closest approachnot earlier than 2033
Distance450 km (280 mi)
InstrumentHeritage InstrumentHeritage Mission
Magnetometer MESSENGER Magnetometer MESSENGER
Narrow-Angle Camera Long Range Reconnaissance Imager (LORRI) New Horizons
Thermal Infrared Camera Diviner Lunar Reconnaissance Orbiter
Langmuir Probe and Waves MAVEN Langmuir Probe and Waves (LPW) MAVEN
Search coil magnetometer TRACERS search coil magnetometer (MSC) TRACERS
Fast imaging plasma spectrometer MESSENGER energetic particle and plasma spectrometer (EPPS)MESSENGER
Electrostatic analyzers Solar Wind Electrons Alphas and Protons (SWEAP) Parker Solar Probe
Energetic Charged Particle Detector EPI-Lo Parker Solar Probe
Visible-Near Infrared Imaging Spectrometer & Wide-angle camera L'Ralph Lucy
Radio Science ExperimentUltraStable Oscillatornone (part of spacecraft communications system)

Atmospheric probe instruments

The atmospheric probe is proposed to carry 4 scientific instruments as part of the baseline concept. [1]

InstrumentHeritage InstrumentHeritage Mission
Double focus mass spectrometer Rosetta Orbiter Spectrometer for Ion and Neutral Analysis (ROSINA) Rosetta
Atmospheric Structure Instrument Huygens Atmospheric Structure Instrument (HASI) Huygens
Ortho-Para H2 Detector(in development) [8] none
Radio Science ExperimentUltraStable Oscillatornone (part of probe communications system)

See also

Uranus mission proposals

Related Research Articles

<i>Voyager 2</i> NASA "grand tour" planetary probe

Voyager 2 is a space probe launched by NASA on August 20, 1977, to study the outer planets and interstellar space beyond the Sun's heliosphere. As a part of the Voyager program, it was launched 16 days before its twin, Voyager 1, on a trajectory that took longer to reach gas giants Jupiter and Saturn but enabled further encounters with ice giants Uranus and Neptune. Voyager 2 remains the only spacecraft to have visited either of the ice giant planets, and was the third of five spacecraft to achieve Solar escape velocity, which allowed it to leave the Solar System.

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

Uranus is the seventh planet from the Sun. It is a gaseous cyan-coloured ice giant. Most of the planet is made of water, ammonia, and methane in a supercritical phase of matter, which in astronomy is called 'ice' or volatiles. The planet's atmosphere has a complex layered cloud structure and has the lowest minimum temperature of 49 K out of all the Solar System's planets. It has a marked axial tilt of 82.23° with a retrograde rotation period of 17 hours and 14 minutes. This means that in an 84-Earth-year orbital period around the Sun, its poles get around 42 years of continuous sunlight, followed by 42 years of continuous darkness.

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

Titania, also designated Uranus III, is the largest of the moons of Uranus and the eighth largest moon in the Solar System at a diameter of 1,578 kilometres (981 mi), with a surface area comparable to that of Australia. Discovered by William Herschel in 1787, it is named after the queen of the fairies in Shakespeare's A Midsummer Night's Dream. Its orbit lies inside Uranus' magnetosphere.

<span class="mw-page-title-main">Ice giant</span> Giant planet primarily consisting of compounds with freezing points exceeding 100°K

An ice giant is a giant planet composed mainly of elements heavier than hydrogen and helium, such as oxygen, carbon, nitrogen, and sulfur. There are two ice giants in the Solar System: Uranus and Neptune.

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.

<span class="mw-page-title-main">Exploration of Uranus</span> Exploration in space

The exploration of Uranus has, to date, been through telescopes and a lone probe by NASA's Voyager 2 spacecraft, which made its closest approach to Uranus on January 24, 1986. Voyager 2 discovered 10 moons, studied the planet's cold atmosphere, and examined its ring system, discovering two new rings. It also imaged Uranus' five large moons, revealing that their surfaces are covered with impact craters and canyons.

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

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.

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

Neptune has been directly explored by one space probe, Voyager 2, in 1989. As of 2024, there are no confirmed future missions to visit the Neptunian system, although a tentative Chinese mission has been planned for launch in 2024. NASA, ESA, and independent academic groups have proposed future scientific missions to visit Neptune. Some mission plans are still active, while others have been abandoned or put on hold.

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

Neptune is the eighth and farthest known planet from the Sun. It is the fourth-largest planet in the Solar System by diameter, the third-most-massive planet, and the densest giant planet. It is 17 times the mass of Earth, and slightly more massive than fellow ice giant Uranus. Neptune is denser and physically smaller than Uranus because its greater mass causes more gravitational compression of its atmosphere. Being composed primarily of gases and liquids, it has no well-defined solid surface. The planet orbits the Sun once every 164.8 years at an orbital distance of 30.1 astronomical units. It is named after the Roman god of the sea and has the astronomical symbol , representing Neptune's trident.

<i>Planetary Science Decadal Survey</i> Publication of the United States National Research Council

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.

<span class="mw-page-title-main">Uranus Pathfinder</span> Space mission concept

Uranus Pathfinder was a mission concept for the Uranian system evaluated in the 2010s by the European Space Agency. In 2011, scientists from the Mullard Space Science Laboratory in the United Kingdom proposed the joint NASA–ESA Uranus Pathfinder mission to Uranus. It would have been a medium-class (M-class) mission to be launched in 2022, and was submitted to the ESA in December 2010 with the signatures of 120 scientists from around the globe. ESA caps the cost of M-class missions at €470 million. Uranus Pathfinder was proposed in support of ESA's Cosmic Vision 2015–2025. The mission study including several possible combinations of launch dates, trajectories, and flybys, including flybys of Earth, Venus, and of the planet Saturn. Indeed, the study noted the velocity change requirements are only marginally higher than for typical missions to Saturn of this period.

<span class="mw-page-title-main">ODINUS</span>

ODINUS is a space mission concept proposed to the European Space Agency's Cosmic Vision programme. The ODINUS mission concept proposes to expand the Uranus orbiter and probe mission to two twin orbiters— dubbed Freyr and Freyja, the twin gods of the Norse pantheon. Their primary mission would be to study Neptune and Uranus with one orbiter each. If selected, ODINUS would launch in 2034.

MUSE is a European proposal for a dedicated mission to the planet Uranus to study its atmosphere, interior, moons, rings, and magnetosphere. It is proposed to be launched with an Ariane 6 in 2026, travel for 16.5 years to reach Uranus in 2044, and would operate until 2050.

The following outline is provided as an overview of and topical guide to Uranus:

<span class="mw-page-title-main">Europa Lander</span> Proposed NASA lander for Europa

The Europa Lander is a proposed astrobiology mission concept by NASA to send a lander to Europa, an icy moon of Jupiter. If funded and developed as a large strategic science mission, it would be launched in 2027 to complement the studies by the Europa Clipper orbiter mission and perform analyses on site.

<span class="mw-page-title-main">Ocean Worlds Exploration Program</span> NASA program for the exploration of water worlds in the Solar System

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.

<span class="mw-page-title-main">OCEANUS</span> Proposed space mission to Uranus

OCEANUS is a mission concept conceived in 2016 and presented in 2017 as a potential future contestant as a New Frontiers program mission to the planet Uranus. The concept was developed by the Astronautical engineering students of Purdue University during the 2017 NASA/JPL Planetary Science Summer School. OCEANUS is an orbiter, which would enable a detailed study of the structure of the planet's magnetosphere and interior structure that would not be possible with a flyby mission.

<span class="mw-page-title-main">Neptune Odyssey</span> NASA orbiter mission concept to study the Neptune system

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.

<span class="mw-page-title-main">Enceladus Orbilander</span> Proposed NASA space probe to Saturns moon Enceladus

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. 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.

References

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