Various Nebulae Stuff (Blender 3D)
i can explain how to make these if anyone's asking. can be pretty heavy to render but it's fiiiine

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Various Nebulae Stuff (Blender 3D)
i can explain how to make these if anyone's asking. can be pretty heavy to render but it's fiiiine

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Hubble's sharpest image of the Orion Nebula with proplyd highlights
Hubble's sharpest image of the Orion Nebula with proplyd highlights
The gorgeous Orion Nebula is home to tens of what could be fledgling planetary systems. In this image, six of these modest "smudges" with big potential are shown (from top down): 132-1832, 206-446, 180-331, 106-417, 231-838 and 181-825.
Within the awe-inspiring, gaseous folds of Orion, researchers have identified two different types of discs around young and forming stars: those that lie close to the brightest star in the cluster (Theta 1 Orionis C) and those farther away from it. This bright star heats up the gas in the nearby discs, causing them to shine brightly. The discs that are farther away do not receive enough of the energetic radiation from the star to set the gas ablaze; thus, they can only be detected as a dark silhouette against the background of the bright nebula, as the dust that surrounds these discs absorbs background visible light. In these silhouetted discs, astronomers are better able to study the properties of the dust grains that are thought to bind together and possibly form planets like our own.
The brighter discs are indicated by a glowing cusp in the excited material and facing the bright star, but which we see at a random orientation within the nebula, so some appear edge on, and others face on, for instance. Other interesting features enhance the look of these captivating objects, such as emerging jets of matter and shock waves. The dramatic shock waves are formed when the stellar wind from the nearby massive star collides with the gas in the nebula, sculpting boomerang shapes or arrows or even, in the case of 181-825, a space jellyfish!
Editor's note (March 2023): The image shown above of proplyd 106-417 (fourth from the top) is mistakenly pointing towards the location of a different proplyd, 244-440. Proplyd 106-417's true location is on other side of the Orion Trapezium, hidden by the image of proplyd 180-331.
Credits
NASA, ESA, M. Robberto (Space Telescope Science Institute/ESA), the Hubble Space Telescope Orion Treasury Project Team and L. Ricci (ESO)
Protoplanetary disc in the Orion Nebula
Disks around young stars (also known as circumstellar or protoplanetary disks) are thought to be made up of 99% gas and 1% dust. Even that small amount of dust is enough to make the disks opaque and dark at visible wavelengths. The dark disk is seen in this image because they are silhouetted against the bright backdrop of the hot gas of the Orion nebula.
Credits
Mark McCaughrean (Max-Planck-Institute for Astronomy), C. Robert O'Dell (Rice University), and NASA/ESA
New Hubble image of Kleinmann-Low Nebula
This composite image of the Kleinmann-Low Nebula, part of the Orion Nebula complex, is composed of several pointings of the NASA/ESA Hubble Space Telescope in optical and near-infrared light. Infrared light allows to peer through the dust of the nebula and to see the stars therein. The revealed stars are shown with a bright red colour in the image.
With this image, showing the central region of the Orion Nebula, scientists were looking for rogue planets and brown dwarfs. As side-effect they found a fast-moving runaway star.
Credits
NASA, ESA/Hubble
Light continues to echo three years after stellar outburst
The Hubble Space Telescope's latest image of the star V838 Monocerotis (V838 Mon) reveals dramatic changes in the illumination of surrounding dusty cloud structures. The effect, called a light echo, has been unveiling never-before-seen dust patterns ever since the star suddenly brightened for several weeks in early 2002.
Credits
NASA, ESA, and The Hubble Heritage Team (AURA/STScI)

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Fonte: nightcafe.art
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Planetary Nebulae Sketches
Next up in my astronomy series of sketches drawn at the eyepiece of a telescope: Planetary Nebulae.
Planetary nebulae were named by William Herschel, the discoverer of the planet Uranus. Through a telescope, Uranus looks like a faint, dim, slightly bluish circle. When he found a class of nebulae that also looked like faint, dim, slightly bluish circles, he was like "hey everyone this reminds me of that planet I found" and called them "Nebulae of Planetary Character."
Planetary Nebulae have nothing to do with planets, but the name stuck. In fact they are dying stars. Spooky. When an old red giant gets really big, and its inside gets really hot, it starts slowly blowing away the outer layers into space. Eventually the hot core is exposed to space, and it's hot enough that it's emitting enough ultraviolet light to cause the ejected gas to glow visibly. This is the fate of our Sun: not a supernova explosion, but a slow casting off of outer layers.
Here are two planetary nebulae visible in the summer sky as seen through a 10" dobsonian reflector telescope: Messier 27 in Vulpecula, and Messier 57 in Lyra. Both of them have very different shapes as a result of their star's rotation axis. With M57 we may be looking at a spherical bubble, or at a pair of cones with the circular side of the cones facing us. With M27 we're looking towards the equator of the former star, where the planetary nebula was formed by emitting plumes of gas primarily out of the polar region of the star, resulting in a two-lobed appearance.
Text transcript and more planetary nebulae sketches below the cut!