direct imaging
(direct detection)
(detection/observation of exoplanets by taking pictures of it)
Direct imaging is a method of discovering and observing extra-solar planets,
but can be done only for nearby stars, planets orbiting far from their
stars (e.g., many AU), and hot (bright) planets and/or cool stars,
such as brown dwarfs. It is merely imaging the planet, but generally
requires specialized methods to avoid the glare of the star, such
as use of a coronagraph. Planets have been observed and
discovered using this technique, for example, around HR 8799.
Such observation is considered necessary for spotting some types
of biosignatures, likely for any that are part of the
planetshine.
The phrase direct imaging is also commonly used for other
challenging-to-image objects such as
protoplanetary disks.
(exoplanets)
Further reading:
https://en.wikipedia.org/wiki/Methods_of_detecting_exoplanets#Direct_imaging
https://en.wikipedia.org/wiki/List_of_directly_imaged_exoplanets
http://www.planetary.org/explore/space-topics/exoplanets/direct-imaging.html
http://www.as.utexas.edu/astronomy/education/sum11/endl/secure/AST_s309_ss11_8.pdf
https://exoplanets.nasa.gov/resources/2286/direct-imaging/
Referenced by pages:
2M1207
51 Eridani b
adaptive optics (AO)
angular differential imaging (ADI)
atmospheric model
BEAST
Beta Pictoris b (β Pic b)
COCONUTS
coronagraph
Darwin
earthshine
Exo-S
exosatellite
extra-solar planet
extreme adaptive optics (ExAO)
HabEx
HD 114762
HD 209458 b
HR 8799
James Webb Space Telescope (JWST)
Lyot coronagraph (CLC)
Magellan Telescopes
orbitize
PALMS
photometry
projected semi-major axis
protoplanetary disk (PPD)
PSF fitting
red dwarf
reference star differential imaging (RDI)
Roman Space Telescope (RST)
speckle suppression
SPECULOOS
SPHERE
Index