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Optical technologies in ESA programmes - Congrex

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The SPICA mission<br />

SPICA = SPace IR telescope for Cosmology & Astrophysics.<br />

•<br />

•<br />

Formation of stars, galaxies, planets, exo-planet characterisation (5 - 210 um).<br />

Astronomical background limited performance, by means of a 5-6K, 3.5m diameter telescope.<br />

JAXA led mission:<br />

• Observatory at L2. Telescope at T=5-6K, �=3.5m M1, cryogens free.<br />

• Phase A study ongo<strong>in</strong>g at JAXA – Launch by 2018, LV=H-IIB.<br />

• Model payload:<br />

• MIR (5-38µm) camera & spectrometer (JAXA).<br />

• MIR (5-27µm) coronograph (JAXA).<br />

• SAFARI (30-210µm) imag<strong>in</strong>g spectrometer (Europe).<br />

• BLISS (sub-mm) spectrometer (US).<br />

Envisaged European contribution:<br />

• Mission of opportunity (large scientific return for < M class cost).<br />

• SPICA Telescope Assembly (STA) � 2x <strong>in</strong>dustrial study (ASF & TAS-F).<br />

• Ground station (4hr/day) � <strong>ESA</strong> assessment.<br />

• SpicA FAR-<strong>in</strong>frared Instrument (SAFARI). Nationally funded � consortium study.<br />

Optics <strong>in</strong> <strong>ESA</strong> <strong>programmes</strong> | Roland Meynart | ICSO �ό��� 2010 | 05 October 2010 | Earth Observation | Slide 46

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