The very faint companion star to Iota Sagitarii seen with SPHERE

The star HR 7581 (Iota Sgr) was observed in SPHERE survey mode (parallel observation in the near infrared with the dual imaging camera [left] and the integral field spectrograph [right]). A very low mass star, more than 4000 times fainter that its parent star, was discovered orbiting Iota Sgr at a tiny separation of 0.24". This is a vital demonstration of the power of SPHERE to image faint objects very close to bright ones.

The bright star itself has been suppressed almost completely by SPHERE, to allow the faint companion to appear as a clear bright spot to the upper right of the centre. This shows the great potential for SPHERE to detect exoplanets.

Autorska prava:

ESO/J.-L. Beuzit et al./SPHERE Consortium

O slici

Datum objavljivanja:4. jun 2014. 12:00
Povezana saopštenja:eso1417
Veličina:574 x 287 px

O objektu

Naziv:HR 7581
Tip:Milky Way : Star

Formati slika

Veliki JPEG
50,2 KB