v0.2 - 25-04-2020
The outer planets are called gas giants. They are Jupiter, Saturn, Uranus and Neptune respectively. So far only one mission, Galileo, dove into the thick atmosphere of these gas giants. The term lander for a gas giant is somewhat abstract as there is no real hard surface to land on, a better term would be "atmospheric probe". However, the moons of gas giants do have a solid surface that can be landed on.
Operator: NASA
Target: Jupiter
Landing date: 2003
Status: Completed
The Galileo atmospheric probe was part of NASA’s 1989 Galileo mission to Jupiter. As part of the mission, a 337kg probe was deployed from the spacecraft tasked with collecting data from the Jovian atmosphere. The probe endured a maximum deceleration of 228g and temperatures in excess of 16,000°C but was still able to transmit useful data for 58 minutes before ultimately succumbing to the intense pressures of Jupiter’s atmosphere.
The probe used a two-stage parachute system to control its descent into the Jovian atmosphere. Shortly after atmospheric entry, once the vehicle had passed the period of maximum heating and deceleration, having burnt off over 100kg of ablator material from the heat shield, the parachute system was activated. First, a pilot chute was deployed from the top of the vehicle using a mortar system. This pilot chute was used to pull off the vehicle's back cover, deploying the 2.47m projected diameter conical ribbon main parachute. This parachute was designed to help control the vehicle's descent rate through the atmosphere rather than to allow the vehicle to land. Finally, the heat shield was jettisoned, exposing the vehicle's sample analysis instruments to the atmosphere and allowing the probe to start transmitting the data it had collected to the orbiter. In order to survive the harsh conditions on Jupiter, the main parachute canopy and suspension lines were made from the temperature-resistant polymer, Dacron, with the parachute riser made from the aramid, Kevlar.
Although the Galileo Jupiter Atmospheric Probe’s mission was relatively short, it gathered a lot of valuable data about Jupiter’s atmosphere. It gave an insight into the composition of the atmosphere and detected winds in excess of 640m/s. [12]
v0.2 - 25-04-2020
Galileo probe during integration
Operator: NASA
Target: Neptune's moon, Triton
Landing date: 2040
Status: Proposed
Although there are a lot of landers going to our nearest neighbours, NASA is also looking further into the solar system with the dragonfly and Triton hopper. These are proposed to go to a moon of Saturn and Neptune, respectively. As the name suggests, the Triton hopper is proposed to land on Triton, one of Neptune’s moons. Although the project is currently in development, it has already completed its phase I study, and a conceptual design was drawn up [99].
When landing on Triton, the Triton hopper would be landing on a moon in a retrograde orbit around its parent planet about 30 AU from the Earth (1AU=distance Earth-Sun). This retrograde orbit is most likely because Triton is a captured object from the Kuiper Belt. Making the Triton hopper the first human-made object to land on a Kuiper belt Object when it would land in 2040 [99].
The vehicle would land using propulsion since the atmosphere on Triton is only 14-40 microbar (~1 Pa), mainly consisting of Nitrogen. To get to the point, a landing can be attempted, the entire system would first be inserted with a solid stage into a 200km parking orbit around Triton. Then the lander would separate and, using a bi-propellant stage would descend to an altitude of 250m, where the hopper would make its first hop to the surface [99].
The Triton Hopper is estimated to have a dry weight of 325kg and 450kg when fully fuelled with Nitrogen. The engine used for hopping would use Nitrogen, which is sourced after the first hop from the atmosphere and surface of Triton because the atmosphere is made mostly of Nitrogen. The hops it would make will be 1.3 km high and 5.2 km downrange, during which it will gather data on the atmosphere of Triton. Besides this, it will take along a wide range of sensors and cameras to analyse and photograph Triton [99].
The Triton hopper
Operator: NASA
Target: Saturn's Moon, Enceladus
Landing date: 2038
Status: Proposed
The Enceladus Orbilander is a proposed NASA Flagship mission aimed at exploring Saturn's moon Enceladus. The mission combines both orbiter and lander functions into a single spacecraft, designed to sample Enceladus' water plumes and study surface materials for evidence of life. The spacecraft, manufactured by APL, is set to launch in October 2038 and will embark on a 15-year journey, including a 7-year cruise, a 4-year tour of Saturn's moons, and a science phase consisting of 1.5 years in orbit around Enceladus followed by 2 years on its surface. Enceladus, known for its active water plumes and subsurface ocean, has been previously studied by the Voyager and Cassini spacecraft, which revealed its geological activity and potential habitability. The mission's estimated cost is $4.9 billion, and it is prioritized as the second highest Flagship mission in the 2023–2032 Planetary Science Decadal Survey. The spacecraft will carry a suite of scientific instruments, including a high-resolution mass spectrometer, electrochemical sensor array, microscope, cameras, and seismometer, tailored to different scientific operations. The mission profile includes a Jupiter flyby in 2040, Saturn orbit insertion in 2045, and a complex tour of Saturn's moons before entering Enceladus orbit and eventually landing on its surface using terrain-relative navigation.
Operator: NASA
Target: Uranus
Landing date: 2045
Status: Proposed
The Uranus Orbiter and Probe mission, operated by NASA, aims to study Uranus and its moons, deploying an atmospheric probe to characterize Uranus's atmosphere. The launch is proposed for the mid to late 2030s using a Falcon Heavy rocket, with a mission duration of 13.4 years for the cruise phase and 4.5 years for the science phase.
The spacecraft has a launch mass of 7,235 kg and a dry mass of 2,756 kg. It includes an orbiter payload of 60.5 kg and an atmospheric probe payload of 19.7 kg. The power source is 735 W from three Next-Generation Radioisotope Thermoelectric Generators.
Key science questions focus on Uranus's origin, interior, and atmosphere, studying atmospheric circulation, 3D structure, formation, evolution, and composition. The mission also investigates the magnetosphere and the internal structures, geological history, compositions, and formation processes of Uranus's satellites and rings.
The atmospheric probe will study the vertical distribution of cloud-forming molecules, thermal stratification, and wind speed as a function of depth. It will carry four scientific instruments: a double focus mass spectrometer, an atmospheric structure instrument, an ortho-para H2 detector, and a radio science experiment. This mission aims to enhance our understanding of Uranus and its system.
2021 sketch of teh Uranus Orbiter and Probe
Operator: NASA
Target: Jupiter's Moon, Europa
Landing date: 2030+
Status: Not selected?
The European lander was a mission proposed by NASA to land and explore the Jovian moon Europa and in support of the Europa Clopper orbiter. The mission was in the end rejected in favor of the Uranus Orbiter and Probe and Enceladus Orbilander. The mission was designed out of multiple modules. The complete stack would be launched on a SLS and fly to Jupiter where it would separate from the “carrier stage”. The entry system would consist of a Deorbit Stage (DOS) and a Powered Descent Vehicle (PDV). The DOS would only ensure the mission dives into the atmosphere after which it is discarded. The PDV consisted of the lander and a sky crane system comparable to the Martian landers. This system would allow for safe landing with about one hundred meters of accuracy.