If you thought Hubble was a complicated project, look
at this deployment animation of the Webb, it'll take
a month to deploy and reach start it's halo orbit
around the L2 point. If they pull it off it'll
be quite an accomplishment.
James Webb Space Telescope Deployment In Detail
https://www.youtube.com/watch?v=bTxLAGchWnA
And the results could be breathtaking, from
the NASA page
Webb And Exoplanets
One of the main uses of the James Webb Space Telescope will be to study
the atmospheres of exoplanets, to search for the building blocks of life
elsewhere in the universe. But Webb is an infrared telescope. How is
this good for studying exoplanets?
One method Webb will use for studying exoplanets is the transit method,
which means it will look for dimming of the light from a star as its
planet passes between us and the star. (Astronomers call this a
"transit".) Collaboration with ground-based telescopes can help us
measure the mass of the planets, via the radial velocity technique
(i.e., measuring the stellar wobble produced by the gravitational tug of
a planet), and then Webb will do spectroscopy of the planet's atmosphere.
Webb will also carry coronagraphs to enable direct imaging of exoplanets
near bright stars. The image of an exoplanet would just be a spot, not a
grand panorama, but by studying that spot, we can learn a great deal
about it. That includes its color, differences between winter and
summer, vegetation, rotation, weather...How is this done? The answer
again is spectroscopy.
+ Sodium in atmosphere of exoplanet HD 209458
The presence of sodium in the atmosphere of Hot Jupiter exoplanet HD
209458 is measured by studying its spectrum. Credit: A. Field, STScI
Spectroscopy
Spectroscopy is simply the science of measuring the intensity of light
at different wavelengths. The graphical representations of these
measurements are called spectra, and they are the key to unlocking the
composition of exoplanet atmospheres.
When a planet passes in front of a star, the starlight passes through
the planet's atmosphere. If, for example, the planet has sodium in its
atmosphere, the spectrum of the star, added to that of the planet, will
have what we call an "absorption line" in the place in the spectra where
would expect to see sodium (see graphic below). This is because
different elements and molecules absorb light at characteristic
energies; and this is how we know where in a spectrum we might expect to
see the signature of sodium (or methane or water) if it is present.
Why is an infrared telescope key to characterizing the atmospheres of
these exoplanets? The benefit of making infrared observations is that it
is at infrared wavelengths that molecules in the atmospheres of
exoplanets have the largest number of spectral features. The ultimate
goal, of course, is to find a planet with a similar atmosphere to that
of Earth.
https://jwst.nasa.gov/origins.html
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>
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