Solar Orbiter
Science & Exploration

Solar Orbiter factsheet

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ESA / Science & Exploration / Space Science / Solar Orbiter

Mission: To study the Sun up close and from high latitudes, providing the first images of the Sun’s poles and investigating the heliosphere

Partnerships: Solar Orbiter is an ESA mission with strong NASA participation

Launch mass: 1800 kg
Science payload mass: 209 kg
Body: 2.5 x 3.1 x 2.7 m
Total length with solar arrays deployed: 18 m
Solar panels: 6, each 2.1 x 1.2 m
Payload power: 180 W
Instrument boom: 4.4 m
3 x radio and plasma wave antennas: 6.5 m each

Solar Orbiter factsheet
Solar Orbiter factsheet

Launch: February 2020
Vehicle: Atlas 5, Cape Canaveral

Flybys: Multiple gravity assists with Venus will increase Solar Orbiter’s inclination out of the plane of the Solar System by 24º (nominal mission) to 33º (extended mission)

Closest approaches: Solar Orbiter will make a close approach of the Sun every six months. Its distance from the Sun varies from within the orbit of Mercury to close to the orbit of Earth

Science instruments
EPD: Energetic Particle Detector – PI: Javier Rodríguez-Pacheco, University of Alcalá, Spain
EUI: Extreme Ultraviolet Imager – PI: Pierre Rochus, Centre Spatial de Liège, Belgium
MAG: Magnetometer– PI: Tim Horbury, Imperial College London, United Kingdom
Metis: Coronagraph – PI: Marco Romoli, INAF – University of Florence, Italy
PHI: Polarimetric and Helioseismic Imager­ – PI: Sami Solanki, Max-Planck-Institut für Sonnensystemforschung, Germany
RPW: Radio and Plasma Waves– PI: Milan Maksimovic, LESIA, Observatoire de Paris, France
SoloHI: Heliospheric Imager – PI: Russell A. Howard, US Naval Research Laboratory, Washington, D.C., USA
SPICE: Spectral Imaging of the Coronal Environment – European-led facility instrument
STIX: X-ray Spectrometer/Telescope­ – PI: Säm Krucker, FHNW, Windisch, Switzerland
SWA: Solar Wind Plasma Analyser – PI: Christopher Owen, Mullard Space Science Laboratory, United Kingdom

Mission facts

  • Solar Orbiter will help us understand how our star creates and controls the giant bubble of plasma that surrounds the whole Solar System and influences the planets within it
  • Solar Orbiter will take the first images of the Sun’s poles from high latitudes
  • Solar Orbiter will combine in situ measurements of the solar wind around the spacecraft with remote sensing, looking at the Sun’s features from afar, to connect the two together
  • At closest approach, Solar Orbiter will be about approximately 42 million kilometres from the Sun
  • The spacecraft has been tested to withstand temperatures up to 500ºC – it will endure thirteen times the amount of solar heating that satellites in Earth’s orbit experience
  • A specially designed black heatshield that will protect the spacecraft and its instruments from the heat of the Sun
  • Solar Orbiter will provide context information for NASA’s Parker Solar Probe, which collects data closer to the Sun, but does not have any Sun-pointing cameras
Solar Orbiter factsheet
Solar Orbiter factsheet

Sun facts

  • Our Sun is one of billions of stars that exist in our Milky Way galaxy
  • The Sun contains 99.9 percent of all matter in our Solar System
  • We live in the extended atmosphere of the Sun, a region of space known as the heliosphere
  • The primary energy the Earth receives from the Sun is light
  • During a single second, the Sun converts four million tonnes of matter into energy
  • The Sun rotates on its axis approximately once every 27 days
  • The Sun’s surface rotates at different speeds in different latitudes. The fastest rotation is at the equator and takes about 25 days; the slowest rotation is at the poles and takes about 36 days
  • The Sun sometimes ejects large packets of plasma from its surface; when directed towards Earth we experience ‘space weather’ which can disrupt satellites and critical infrastructure like power grids