EChO

Source: Wikipedia, the free encyclopedia.
EChO
Mission type
ESA
Websitesci.esa.int/echo
Mission duration4–5 years[1][2]
Spacecraft properties
Launch mass2,100 kg (4,600 lb)[3]
Start of mission
Launch date2024
Kourou ELS[3]
ContractorArianespace
Orbital parameters
Reference system
Sun–Earth L2[2][3]
RegimeHalo or Lissajous
Epochplanned
Main telescope
TypeCassegrain[2]
Diameter1.4 m (4.6 ft)[2]
Focal length2 m (6.6 ft)[2]
Collecting area14 m2 (150 sq ft)[2]
Wavelengthsfrom 0.55 µm (orange)
to 11µm (long-infrared)
(goal: 0.4 to 16 µm)[1][2]
 

The Exoplanet Characterisation Observatory (EChO) was a proposed space telescope[2] as part of the Cosmic Vision roadmap of the European Space Agency, and competed with four other missions for the M3 slot in the programme. On 19 February 2014 the PLATO mission was selected in place of the other candidates in the programme, including EChO.[4]

EChO would have been the first dedicated mission to investigate exoplanetary atmospheres, addressing the suitability of those planets for life and placing the Solar System in context. EChO was intended to provide high resolution, multi-wavelength spectroscopic observations. It would have measured the atmospheric composition, temperature and albedo of a representative sample of known exoplanets, constrain models of their internal structure and improve understanding of how planets form and evolve.[5] It would have orbited around the L2 Lagrange point, 1.5 million km from Earth in the anti-sunward direction.

SPEChO

Following PLATO's M3 selection, a proposal to add EChO on the joint Japanese-European

MIRI (Mid-Infrared Instrument), therefore SPEChO's advantages over other instruments has become a focus of whether or not to include it on SPICA.[6][9]

Other M3 mission candidates

References

  1. ^
    ESA
    . 16 December 2013. Retrieved 28 January 2014.
  2. ^
    S2CID 118578814. Archived from the original
    (PDF) on 2017-09-22. Retrieved 2018-10-23.
  3. ^
    ESA
    . 30 June 2013. Retrieved 28 January 2014.
  4. ^ "ESA selects planet-hunting PLATO mission". ESA. 19 February 2014. Retrieved 20 March 2014.
  5. ^ Tinetti, G.; Cho, J. Y. K.; Griffith, C. A.; Grasset, O.; Grenfell, L.; Guillot, T.; Koskinen, T. T.; Moses, J. I.; Pinfield, D.; Tennyson, J.; Tessenyi, M.; Wordsworth, R.; Aylward, A.; Van Boekel, R.; Coradini, A.; .
  6. ^ a b c "SPICA計画の経緯・現状" (PDF) (in Japanese). Japan Radio Astronomy Forum. 28 January 2015. Archived from the original (PDF) on 2017-01-03. Retrieved 2017-01-03.
  7. Institute for the Physics and Mathematics of the Universe
    . 5 June 2015. Retrieved 2017-01-03.
  8. ^ "SPICAサイエンス検討中間報告" (PDF) (in Japanese). Group of Optical and Infrared Astronomers SPICA task force. 26 November 2014. Retrieved 2017-01-03.
  9. ^ "タスクフォースからの提言 近傍銀河および星惑星系形成分野" (PDF) (in Japanese). Group of Optical and Infrared Astronomers SPICA task force. 26 November 2014. Retrieved 2017-01-03.

External links

This page is based on the copyrighted Wikipedia article: EChO. Articles is available under the CC BY-SA 3.0 license; additional terms may apply.Privacy Policy