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Protoplanetary Disks. By R. Hurt (NASA/JPL-Caltech/IPAC)

Protoplanetary Disk

A protoplanetary disk is a rotating circumstellar disk of dense gas and dust surrounding a young newly formed star, a T Tauri star. The protoplanetary disk may also be considered an accretion disk for the star itself, because gasses or other material may be falling from the inner edge of the disk onto the surface of the star. But this process should not be confused with the accretion process thought to build up the planets themselves.

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Binary Star. By NASA/JPL-Caltech/Univ. of Ariz.

Binary Star

A binary star is a star system consisting of two stars orbiting around their common barycenter. Systems of two, three, four, or even more stars are called multiple star systems. These systems, especially when more distant, often appear to the unaided eye as a single point of light, and are then revealed as double (or more) by other means. Research over the last two centuries suggests that half or more of visible stars are part of multiple star systems.

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Radiotelescopes. By ESO/C. Malin, modified by Krischan

Search for Extraterrestrial Intelligence (SETI)

The search for extraterrestrial intelligence (SETI) is a collective term for the scientific search for intelligent extraterrestrial life. For example, monitoring electromagnetic radiation for signs of transmissions from civilizations on other worlds. There are great challenges in searching the universe for signs of intelligent life, including their identification and interpretation. As various SETI projects have progressed, some have criticized early claims by researchers as being too “euphoric”.

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Gravity Demo. By Krischan

Gravity Demo

A simple 3D demo of gravitation in minib3d. Two bodies with different masses affect each other using Newton’s law of universal gravitation formula which is F=G*((M1*M2)/r²). Includes a single surface path visualization using quads to see the objects gravitation influence. In this demo I’ve used the mass of our sun for the star and the mass of our planet. You can interact with some keys, use the mouse to rotate and zoom the scene.Read More

Wolf-Rayet Star. By ESA/Hubble & NASA Acknowledgement: Judy Schmidt

Wolf-Rayet Star

Wolf-Rayet stars (often referred to as WR stars) are a heterogeneous set of stars with unusual spectra showing prominent broad emission lines of highly ionised helium and nitrogen or carbon. The spectra indicate very high surface temperatures of 30,000 – 200,000 Kelvin, surface enhancement of heavy elements, and strong stellar winds.

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