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But the VLT view, which was obtained using an instrument called SPHERE (short for "Spectro-Polarimetric High-contrast Exoplanet Research"), adds something different and more detailed: a twist in those spiral arms. This twist likely pinpoints the spot where the exoplanet is taking shape, researchers report in a new study describing the observations.
"The twist is expected from some theoretical models of planet formation," study co-author Anne Dutrey, of the Astrophysics Laboratory of Bordeaux in France, said in a statement.
"It corresponds to the connection of two spirals — one winding inwards of the planet's orbit, the other expanding outwards — which join at the planet location," Dutrey said. "They allow gas and dust from the disk to accrete onto the forming planet and make it grow."
www.space.com...
I also know that no telescope can take a picture like the one that they posted in that little video.
originally posted by: gortex
a reply to: rickymouse
I also know that no telescope can take a picture like the one that they posted in that little video.
Radio telescopes can , the picture isn't an optical image.
originally posted by: rickymouse
I also know that no telescope can take a picture like the one that they posted in that little video. It is a computer generated interpretation of what is going on
originally posted by: wildespace
originally posted by: rickymouse
I also know that no telescope can take a picture like the one that they posted in that little video. It is a computer generated interpretation of what is going on
Actually, it's pretty much a straightforward optical image, albeit using adaptive optics and polarising filters. The image comes from the Spectro-Polarimetric High-Contrast Exoplanet Research (SPHERE) camera. It provides direct imaging as well as spectroscopic and polarimetric characterization of exoplanet systems. The instrument operates in the visible and near infrared, achieving, albeit over a limited field of view, superior image quality and contrast for bright targets.
SPHERE comprises the following subsystems:
# The Common Path and Infrastructure (CPI) is the main optical bench. It receives direct light from the telescope, and passes on stabilized, active-optics-corrected, and coronagraph-filtered beams to the three sub-instruments.
# The Integral Field Spectrograph (IFS) covers a 1.73" x 1.73" field of view, translating the spectral data into a three-dimensional (x,y,λ) data cube.
# The Infrared Dual-band Imager and Spectrograph (IRDIS) has a field of view of 11" x 12.5" with a pixel scale of 12.25 mas (milliarcsecond). IRDIS can provide classical imaging. Alternatively, it can be configured to provide simultaneous dual-band imaging using two different narrow bandpass filters targeting different spectral features, or it can be configured to provide simultaneous imaging from two crossed polarizers. When operating in long slit spectroscopy mode (LSS), a coronagraphic slit replaces the coronagraph mask.
# The Zurich Imaging Polarimeter (ZIMPOL) is a high contrast imaging polarimeter operating at the visual and infrared wavelengths, capable of achieving less than 30 mas resolution. It is also capable of diffraction limited classical imaging.