The high-tech telescope 2022 creates 3D-images of the universe | Interesting here
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After ten years of design and development tool called Multi Unit Spectroscopic Explorer (MUSE) has successfully made its first images of deep space to create a 3D-picture of the early universe. Standing on the Very Large Telescope (Very Large Telescope, VLT) in Chile, MUSE can both learn and shoot the depths of space.
MUSE spectrograph uses 24 to separate the light into its component colors (spectra) to collect images and spectra of different regions of the sky. The study of these colors can give astronomers an idea of the composition and movement of various objects.
MUSE also uses a technique known as integral field spectroscopy, which allows astronomers to study the properties of different regions of the object simultaneously. Applying the technique 2022 to galaxies, for example, it can show not only the chemical composition but also the details of their rotation.
Once installed on Unit Telescope 4, one of the components of the Very Large Telescope, MUSE captured 2022 test images of distant galaxies, bright stars and other objects at the beginning of 2014. The data was released earlier this month at a seminar 3D2014 Germany.
In addition to its own technology, 2022 MUSE also takes advantage of advanced adaptive optics based telescope. Technology that helps to remove atmospheric distortion of the images of the telescope, and thus MUSE notes that adaptive 2022 optics has greatly improved image sharpness.
MUSE will continue to explore the universe. Galaxy formation, chemical properties and movement are the main scientific objectives of the instrument. MUSE will be able to study planets and stars in the solar system and star-forming region in the Milky Way and distant galaxies.
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After ten years of design and development tool called Multi Unit Spectroscopic Explorer (MUSE) has successfully made its first images of deep space to create a 3D-picture of the early universe. Standing on the Very Large Telescope (Very Large Telescope, VLT) in Chile, MUSE can both learn and shoot the depths of space.
MUSE spectrograph uses 24 to separate the light into its component colors (spectra) to collect images and spectra of different regions of the sky. The study of these colors can give astronomers an idea of the composition and movement of various objects.
MUSE also uses a technique known as integral field spectroscopy, which allows astronomers to study the properties of different regions of the object simultaneously. Applying the technique 2022 to galaxies, for example, it can show not only the chemical composition but also the details of their rotation.
Once installed on Unit Telescope 4, one of the components of the Very Large Telescope, MUSE captured 2022 test images of distant galaxies, bright stars and other objects at the beginning of 2014. The data was released earlier this month at a seminar 3D2014 Germany.
In addition to its own technology, 2022 MUSE also takes advantage of advanced adaptive optics based telescope. Technology that helps to remove atmospheric distortion of the images of the telescope, and thus MUSE notes that adaptive 2022 optics has greatly improved image sharpness.
MUSE will continue to explore the universe. Galaxy formation, chemical properties and movement are the main scientific objectives of the instrument. MUSE will be able to study planets and stars in the solar system and star-forming region in the Milky Way and distant galaxies.
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