BLOG #2 JPL Innovation

           Humans have always been intrigued by the stars glowing above in the heavens throughout our history, but our contemporary interest in faraway light sources and ‘exoplanets’ consists of a lot more than just primal fascination. Scientists and researchers at NASA and JPL have been on the hunt for exoplanets, or planets that orbit around a star much like our own sun and Earth. The search is for a ‘habitable’ environment, where the atmosphere is not too hot and not too cold and could sustain water, promoting the growth and existence of life!
Obviously, there are numerous technical feats and challenges to overcome in order to locate such planets and simply photographing them proves to be enough of an obstacle in itself. Originally, researchers could detect orbiting planets like our own Earth while studying stars in deep space with space telescopes such as the HUBBLE. The telescope would have internal adjustments and additions made, such as an internal coronagraph which consisted of numerous mirrors and filters to help decrease the amount of flare from starlight in the photographs. This would help the telescope see the area surrounding the star without the star blowing out the photograph. This internal technology allowed HUBBLE to thus detect variations in starlight intensity when a planet would orbit around the star between the telescope and the star itself, very partially eclipsing the star. Although it was the only method NASA had to detect exoplanets, it is not the most efficient process considering the complexity of internal coronagraphs along with the cost, only complicating the already impressive space telescopes.
The next generation of exoplanet discovery comes from the research and technical production of JPL’s lead engineer, Dr. Stuart Shaklan, who is working on a new procedure with JPL’s engineer team for photographing orbiting planets utilizing what JPL calls a “Star Shade”. This Star shade is a physically deployable device capable of eclipsing a star’s intense light emission, allowing high quality, clean photographs to be taken of a star’s surrounding environment. In theory, the star shade would be completely collapsible allowing it to fit into a rocket or telescope, and would then detach and unfold to be the approximate size of a baseball diamond.








The shade would have miniature thrusters attached along with the ability to communicate with the accompanying telescope in order to maintain proper alignment between the telescope, the star shade, and the star.



 The star shade would float approximately 50,000 km away from the telescope in order to achieve a dark enough shadow between the shade and the telescope, allowing flare free photography of the star. Another compelling feature of the star shade itself are its flower petal-like protrusions from its center. These petals serve to greatly decrease the amount of diffraction produced from the starlight behind the shade.





If the star shade were perfectly circular, the light from the star would bend around the round contours of the circular shade and bleed into the photograph, providing unusable results. Thus, a flower petal was devised, muting the amount of diffraction and reducing the amount of stray light entering the imaging sensor.
References:
https://science.nasa.gov/technology/technology-stories/starshade-enable-first-images-earth-sized-exoplanets


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