The Iris Nebula | Astrophotography Tips and Advice for Capturing a Reflection Nebula
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IRIS • Sun’s Swirling Spicules 8.5.2021 • Here we see the surface of our star and solar spicules appear and dissapear as IRIS images gradually higher wavelengths (angstroms 2794A - 2804A) and associated temperature of the solar chromosphere, the interface between the photosphere and corona.. Taken by the IRIS (NASA’s Interface Region Imaging Spectrograph) satellite on 6.5.2021 at 22:49 Solar spicules, originally discovered by Father Secchi in 1877, are small-scale (~200-500 km wide) magnetized g
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La Nebulosa Iris: un Laboratorio de Polvo Perfecto en el Cielo. El polvo cósmico puede resultar un obstáculo para los astrónomos, porque las cámaras que utilizan luz visible no pueden ver a través de él. Sin embargo, estudiar el polvo cósmico en detalle ayuda a los astrónomos a precisar los ingredientes de la cruda mezcla que finalmente da origen a las estrellas. Esta área de la gran Nebulosa Iris, parece estar obstruida por polvo cósmico. Con la brillante luz de la cercana estrella 'HD 200775'
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Granulation Observed with IRIS at 283.2 nm 5.1.2021 • IRIS was designed to observe the Solar chromosphere and transition region; the part of the solar atmosphere between the surface, the photosphere, and the hot corona. An exception is found when looking far into the wings of the Mg II h and k spectral lines, where the photosphere can be observed as well, as shown in this movie. There we see granulation, the result of heat bubbling up from the solar interior (the average size of each granule is
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NASA's IRIS Spots its Biggest Solar Flare Yet
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gizmodo.com
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