Gravity assist 2026-11-05
A gravity assist is a spacecraft flyby that uses the gravity of a moving planet or other massive body to change the spacecraft's trajectory and its orbital energy relative to another body, such as the Sun. In the ideal unpowered two-body encounter, the incoming and outgoing speeds far from the planet are equal in the planet's reference frame. Their directions differ. Adding the planet's motion converts that directional change into a possible speed change in the Sun's reference frame.[ref]
Basics of Spaceflight: A Gravity Assist Primer by NASA. planet-relative incoming/outgoing velocity vectors and planetary-motion vector
Write the planet's nearly constant velocity during the encounter as , and the incoming and outgoing planet-relative velocities as and . Then , , and . Subtracting the squared speeds gives the local change in specific orbital energy:For a hypothetical turn, choose , and , all in . Planet-relative speed stays , while Sun-relative speed changes from to . The specific-energy gain is . Whether a given turn is physically available depends on the planet's mass, the incoming speed and the permitted closest approach.
Conservation of energy is maintained because the planet and spacecraft exchange momentum and energy. The planet's change is extremely small because of its much greater mass. A different encounter geometry can remove orbital energy or mainly change orbital inclination; Ulysses spacecraft used the latter possibility to reach high solar latitudes.[ref]
Gravity Assists for Cassini by NASA. three-body interpretation and conservation-of-energy discussion
Ion propulsion 2026-11-05
Ion propulsion produces thrust by using electrical energy to accelerate ions out of a spacecraft. In a gridded ion engine, a discharge creates ions from propellant such as xenon, electric fields accelerate them through grids, and a neutralizer supplies electrons so the departing beam does not leave the spacecraft progressively charged. The exhaust carries momentum; no surrounding air is required.[ref]
For an ideal directed exhaust with mass flow rate and exhaust velocity , neglecting the pressure term,Here is electrical input power and the fraction converted into directed exhaust kinetic energy. Thus high exhaust speed saves propellant for a given momentum change but reduces thrust at fixed power. At , and , the ideal thrust is .
Ground tests operate the engine in a pumped vacuum chamber, measuring beam current, power, propellant flow and thrust. A bright plume alone cannot establish efficiency or delivered impulse. NASA's Deep Space 1 and Dawn missions demonstrated sustained ion propulsion in flight, where small thrust accumulated over long operating times.[ref]
Microgravity 2026-11-05
Microgravity is a condition of very small residual acceleration or apparent weight experienced within an experimental system. An orbiting spacecraft and its freely moving contents fall together under gravity, greatly reducing the support forces experienced on the ground. A drop tower provides a shorter interval using the same free fall principle.[ref]
Zero Gravity Research Facility by NASA. Free-fall microgravity and experimental facility
Residual disturbances include air resistance, vibrations, vehicle manoeuvres and spatial variation in gravitational acceleration. Their importance depends on the experiment's duration and length scale. Suppressing gravity-driven convection or settling lets surface tension, diffusion and other processes become easier to isolate; the result is an experimentally controlled change in dominant forces, rather than removal of the gravitational field.
Solar Orbiter 2026-11-05
Solar Orbiter is an ESA-led spacecraft with strong NASA participation, launched in February 2020 to connect observations of the Sun with measurements of the solar wind. Its heliocentric orbit and gravity assists allow observations from different distances and increasing solar latitudes, rather than restricting every view to the plane from which Earth sees the Sun.[ref]
Solar Orbiter factsheet by ESA. Mission, Partnerships and Journey
Its ten instruments divide into six for remote sensing and four for sampling the surrounding environment. The remote sensing instruments observe emitted or scattered light from the Sun and its surroundings. The local instruments measure plasma, energetic particles, electric fields, magnetic fields and waves. A magnetometer and particle analysers therefore answer different questions from an image: one measures conditions at the spacecraft, while the other helps locate the remote source.[ref]
Solar Orbiter Mission by the US Naval Research Laboratory. instrument division and lists; physical connectivity between Sun and solar wind
A scientific comparison can ask whether a feature observed near the Sun is associated with a later change in the velocity distribution or composition of locally sampled particles. Identifying the connection requires accounting for the material's travel time and the changing geometry; simultaneous timestamps alone do not establish a common origin. The mission's combined apparatus makes such tests possible. A 2024 analysis, for example, separated proton and alpha particle populations in its solar wind data rather than representing all ions by one mean speed.[ref]
Voyager 1 Created 2026-10-24 Updated 2026-11-05
Voyager 1 is a spacecraft launched on 5 September 1977 to investigate the outer Solar system. It flew past Jupiter in March 1979 and Saturn in November 1980, then continued outward on an extended mission to study the environment beyond the planets.[ref]
Voyager 1 Mission Overview by NASA. Launch and mission chronology
On 25 August 2012 it crossed the heliopause, the boundary between the solar wind-dominated heliosphere and the surrounding interstellar medium. This boundary concerns the plasma environment; it is not a boundary beyond which the Sun's gravity vanishes. Its scientific instruments include detectors of charged particles, a magnetometer and a Voyager plasma-wave instrument. Together, measurements of particles, magnetic fields and plasma waves allow a moving probe to investigate a remote environment that cannot be sampled in a terrestrial laboratory.[ref]
Voyager 1 Mission Overview by NASA. Interstellar mission and science instruments
Voyager 2 2026-11-05
Voyager 2 is a robotic spacecraft launched on 20 August 1977 to investigate the outer Solar system. Its encounters with Jupiter in 1979, Saturn in 1981, Uranus in 1986 and Neptune in 1989 made one mission a comparative study of four giant planets. A gravity assist changes the spacecraft's trajectory and energy relative to the Sun by exchanging momentum with a moving planet, allowing a sequence of encounters that would require much more onboard propulsion if accomplished by engine firings alone.[ref]
Voyager 2 Mission Overview by NASA. launch, mission history and planetary encounter chronology
Voyager 2 later sampled the transition from the solar wind to the surrounding interstellar plasma. On 5 November 2018, its plasma instrument recorded a steep decline in the outward solar wind flow. The instrument inferred plasma properties from electrical currents collected from particles arriving in different directions. Changes in energetic-particle measurements supplied independent evidence: particles associated with the heliosphere declined while galactic cosmic rays became more prominent. The combined observations identify the heliopause crossing, rather than defining the boundary by a predetermined distance.[ref]
NASA's Voyager 2 Probe Enters Interstellar Space by NASA Jet Propulsion Laboratory. 10 December 2018 announcement; plasma-current and particle measurements dating the crossing to 5 November
This is a moving-laboratory experiment: the apparatus travels through regions that cannot be sampled from Earth, while several instruments test the interpretation of a sharp change. Crossing the heliopause means leaving the region dominated by the Sun's outward-flowing plasma; solar gravity does not suddenly end there. The crossing date and the December announcement date are different events.