OCEANUS

Last updated
OCEANUS (Origins and Composition of the Exoplanet Analog Uranus System)
Uranus Voyager2 color calibrated.png
Uranus, an ice giant planet, was photographed in real color by Voyager 2 in January 1986
Mission typeReconnaissance
Operator NASA/JPL
Mission duration≥1.5 years [1]
Spacecraft properties
Launch mass≈3,939 kg
BOL mass ≈2,000 kg [1]
Dry mass≈1,110 kg
Power290 W [1]
Start of mission
Launch date2030 (suggested)
Rocket Atlas V 511 or SLS
Uranus orbiter
Orbital insertion2041
Orbits≥14 (proposed) [1]

OCEANUS (Origins and Composition of the Exoplanet Analog Uranus System) 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. [2] [1] The concept was developed in a different form 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. [2]

Contents

Because of the required technology development and planetary orbital dynamics, the concept suggests a launch in August 2030 on an Atlas V 511 rocket and entering Uranus' orbit in 2041. [1]

Overview

Atlas V, proposed for OCEANUS, shown here launching the Lunar Reconnaissance Orbiter into space Atlas V(401) launches with LRO and LCROSS cropped.jpg
Atlas V, proposed for OCEANUS, shown here launching the Lunar Reconnaissance Orbiter into space

Ice giant sized planets are the most common type of planet according to Kepler data. The little data available on Uranus, an ice giant planet, come from ground-based observations and the single flyby of the Voyager 2 spacecraft, so its exact composition and structure are essentially unknown, as are its internal heat flux, and the causes of its unique magnetic fields and extreme axial tilt or obliquity, [1] making it a compelling target for exploration according to the Planetary Science Decadal Survey. [2] [3] The primary science objectives of OCEANUS are to study Uranus' interior structure, magnetosphere, and the Uranian atmosphere. [1]

The required mission budget is estimated at $1.2 billion. [1] The mission concept has not been formally proposed to NASA's New Frontiers program for assessment and funding. The mission is named after Oceanus, the Greek god of the ocean; he was son of the Greek god Uranus. [4]

Power and propulsion

Since Uranus is extremely distant from the Sun (20 AU), and relying in solar power is not possible past Jupiter, the orbiter is proposed to be powered by three multi-mission radioisotope thermoelectric generators (MMRTG), [2] [1] a type of radioisotope thermoelectric generator. As of 2015, there was enough plutonium available to NASA to fuel three more MMRTG like the one used by the Curiosity rover, one of which was already committed to the Perseverance rover. [5] [6] The other two have not been assigned to any specific mission or program, [6] and could be available by late 2021. [5] A second possible option for powering the spacecraft other than a plutonium powered RTG would be a small nuclear reactor powered by uranium, such as the Kilopower system in development as of 2019.

The trajectory to Uranus would require a Jupiter gravity assist, but such alignments are calculated to be rare in the 2020s and 2030s, so the launch windows will be scant and narrow. [2] To overcome this problem two Venus gravity assists (in November 2032 and August 2034) and one Earth gravity assist (October 2034) are planned along with the use of solar-electric propulsion within 1.5 AU. [1] The science phase would take place from a highly elliptical orbit and perform a minimum of 14 orbits. [1] If launching in 2030, reaching Uranus would occur 11 years later, in 2041, [1] and it would use two bipropellant engines for orbital insertion. [1]

Alternatively, the SLS rocket could be used for a shorter cruise time, [7] but it would result in a faster approach velocity, making orbit insertion more challenging, especially since the density of Uranus' atmosphere is unknown to plan for safe aerobraking. [6]

Payload

Schematic of the OCEANUS probe OCEANUS.jpg
Schematic of the OCEANUS probe

The 12.5 kg scientific payload would include instruments for a detailed study of the magnetic fields and to determine Uranus' global gravity field: [2] [1]

See also

Uranus mission proposals

Related Research Articles

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

Umbriel is the third-largest moon of Uranus. It was discovered on October 24, 1851, by William Lassell at the same time as neighboring moon Ariel. It was named after a character in Alexander Pope's 1712 poem The Rape of the Lock. Umbriel consists mainly of ice with a substantial fraction of rock, and may be differentiated into a rocky core and an icy mantle. The surface is the darkest among Uranian moons, and appears to have been shaped primarily by impacts. However, the presence of canyons suggests early endogenic processes, and the moon may have undergone an early endogenically driven resurfacing event that obliterated its older surface.

<i>Voyager 2</i> First spacecraft to visit Uranus and Neptune (launched in 1977 by NASA)

Voyager 2 is a space probe launched by NASA on August 20, 1977, as a part of the Voyager program. It was launched on a trajectory towards the gas giants Jupiter and Saturn and enabled further encounters with the ice giants Uranus and Neptune. It 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 will allow it to leave the Solar System. Launched 16 days before its twin Voyager 1, the primary mission of the spacecraft was to study the outer planets and its extended mission is to study interstellar space beyond the Sun's heliosphere.

<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 astronomy calls "ice" or volatiles. The planet's atmosphere has a complex layered cloud structure and has the lowest minimum temperature 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 moon of Uranus. At a diameter of 1,578 kilometres (981 mi) it is the eighth largest moon in the Solar System, 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's magnetosphere.

<i>MESSENGER</i> NASA mission to Mercury

MESSENGER was a NASA robotic space probe that orbited the planet Mercury between 2011 and 2015, studying Mercury's chemical composition, geology, and magnetic field. The name is a backronym for "Mercury Surface, Space Environment, Geochemistry, and Ranging", and a reference to the messenger god Mercury from Roman mythology.

<span class="mw-page-title-main">Discovery Program</span> Ongoing solar system exploration program by NASA

The Discovery Program is a series of Solar System exploration missions funded by the U.S. National Aeronautics and Space Administration (NASA) through its Planetary Missions Program Office. The cost of each mission is capped at a lower level than missions from NASA's New Frontiers or Flagship Programs. As a result, Discovery missions tend to be more focused on a specific scientific goal rather than serving a general purpose.

<span class="mw-page-title-main">Moons of Uranus</span> Natural satellites of the planet Uranus

Uranus, the seventh planet of the Solar System, has 28 confirmed moons. Most of them are named after characters that appear in, or are mentioned in, the works of William Shakespeare and Alexander Pope. Uranus's moons are divided into three groups: thirteen inner moons, five major moons, and ten irregular moons. The inner and major moons all have prograde orbits and are cumulatively classified as regular moons. In contrast, the orbits of the irregular moons are distant, highly inclined, and mostly retrograde.

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 Jupiter</span> Overview of the exploration of Jupiter the planet and its moons

The exploration of Jupiter has been conducted via close observations by automated spacecraft. It began with the arrival of Pioneer 10 into the Jovian system in 1973, and, as of 2024, has continued with eight further spacecraft missions in the vicinity of Jupiter and two more en route. All but one of these missions were undertaken by the National Aeronautics and Space Administration (NASA), and all but four were flybys taking detailed observations without landing or entering orbit. These probes make Jupiter the most visited of the Solar System's outer planets as all missions to the outer Solar System have used Jupiter flybys. On 5 July 2016, spacecraft Juno arrived and entered the planet's orbit—the second craft ever to do so. Sending a craft to Jupiter is difficult, mostly due to large fuel requirements and the effects of the planet's harsh radiation environment.

<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 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">Advanced Stirling radioisotope generator</span>

The advanced Stirling radioisotope generator (ASRG) is a radioisotope power system first developed at NASA's Glenn Research Center. It uses a Stirling power conversion technology to convert radioactive-decay heat into electricity for use on spacecraft. The energy conversion process used by an ASRG is significantly more efficient than previous radioisotope systems, using one quarter of the plutonium-238 to produce the same amount of power.

<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. Compared to its fellow ice giant Uranus, Neptune is slightly more massive, but denser and smaller. Being composed primarily of gases and liquids, it has no well-defined solid surface, and 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.

<span class="mw-page-title-main">Uranus Orbiter and Probe</span> Proposed NASA space mission to Uranus

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.

<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.

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.

<span class="mw-page-title-main">Jessica Watkins</span> American astronaut (born 1988)

Jessica Andrea Watkins is an American NASA astronaut, geologist, aquanaut and former international rugby player. Watkins was announced as the first Black woman who completed an International Space Station long-term mission in April 2022. On June 9, 2022, at 7:38 UTC, she became the African American woman with the most time in space, surpassing Stephanie Wilson's 42 day, 23 hour and 46 minute record.

<span class="mw-page-title-main">Oceanus (Titan orbiter)</span> 2017 proposed NASA Triton orbiter space probe

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.

FIRE is a concept mission to Jupiter's innermost major moon Io. The mission was first presented in 2012 for a possible future consideration by NASA's New Frontiers program.

<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.

References

  1. 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 Bramson, A. M; Elder, C. M; Blum, L. W; Chilton, H. T; Chopra, A; Chu, C; Das, A; Delgado, A; Fulton, J; Jozwiak, L; Khayat, A; Landis, M. E; Molaro, J. L; Slipski, M; Valencia, S; Watkins, J; Young, C. L; Budney, C. J; Mitchell, K. L (2017). "OCEANUS: A Uranus Orbiter Concept Study from the 2016 NASA/JPL Planetary Science Summer School". 48th Lunar and Planetary Science Conference. 48 (1964): 1583. Bibcode:2017LPI....48.1583B.
  2. 1 2 3 4 5 6 7 Elder, C. M; Bramson, A. M; Blum, L. W; Chilton, H. T; Chopra, A; Chu, C; Das, A; Davis, A; Delgado, A; Fulton, J; Jozwiak, L; Khayat, A; Landis, M. E; Molaro, J. L; Slipski, M; Valencia, S; Watkins, J; Young, C. L; Budney, C. J; Mitchell, K. L (2017). "New Frontiers-Class Missions to the Ice Giants". Planetary Science Vision 2050 Workshop. 1989: 8147. Bibcode:2017LPICo1989.8147E.
  3. "Lean U.S. missions to Mars, Jupiter moon recommended". 7 March 2011. Reuters. 8 March 2011.
  4. OCEANUS: A Concept Study (PDF) – poster. 2017.
  5. 1 2 Leone, Dan (11 March 2015). "U.S. Plutonium Stockpile Good for Two More Nuclear Batteries after Mars 2020". Space News. Retrieved 12 March 2015.
  6. 1 2 3 Moore, Trent (12 March 2015). "NASA can only make three more batteries like the one that powers the Mars rover". Blastr. Archived from the original on 14 March 2015. Retrieved 13 March 2015.
  7. Mansell, J; Kolencherry, N; Hughes, K; Arora, A; Chye, H.S; Coleman, K; Elliott, J; Fulton, S; Hobar, N; Libben, B; Lu, Y; Millane, J; Mudek, A; Podesta, L; Pouplin, J; Shibata, E; Smith, G; Tackett, B; Ukai, T; Witsberger, P; Saikia, S (2017). "Oceanus: A multi-spacecraft flagship mission concept to explore Saturn and Uranus". Advances in Space Research. 59 (9): 2407–33. Bibcode:2017AdSpR..59.2407M. doi:10.1016/j.asr.2017.02.012.