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  2. Interstellar cloud - Wikipedia

    en.wikipedia.org/wiki/Interstellar_cloud

    An interstellar cloud is generally an accumulation of gas, plasma, and dust in our and other galaxies. But differently, an interstellar cloud is a denser-than-average region of the interstellar medium , the matter and radiation that exists in the space between the star systems in a galaxy.

  3. Pillars of Creation - Wikipedia

    en.wikipedia.org/wiki/Pillars_of_Creation

    This video clip shows a visualization of the three-dimensional structure of the Pillars of Creation. Closer view of one pillar. Pillars of Creation is a photograph taken by the Hubble Space Telescope of elephant trunks of interstellar gas and dust in the Eagle Nebula, in the Serpens constellation, some 6,500–7,000 light-years (2,000–2,100 pc; 61–66 Em) from Earth. [1]

  4. Nebular hypothesis - Wikipedia

    en.wikipedia.org/wiki/Nebular_hypothesis

    The visible-light (left) and infrared (right) views of the Trifid Nebula—a giant star-forming cloud of gas and dust located 5,400 light-years away in the constellation Sagittarius Stars are thought to form inside giant clouds of cold molecular hydrogen — giant molecular clouds roughly 300,000 times the mass of the Sun ( M ☉ ) and 20 ...

  5. GUSTO (telescope) - Wikipedia

    en.wikipedia.org/wiki/GUSTO_(telescope)

    An artist's concept of the GUSTO mission gondola carrying the telescope, cryocoolers, and solar panels. Mass is about 2 tons. GUSTO (Galactic / Extragalactic ULDB Spectroscopic Terahertz Observatory) is a high-altitude balloon mission that carries an infrared telescope to measure fine-structure line emission from the interstellar medium.

  6. Origins Space Telescope - Wikipedia

    en.wikipedia.org/wiki/Origins_Space_Telescope

    Diagram of the envisioned mirror diameter of the Origins Space Telescope. [7]The Roadmap envisaged a mid- to far-infrared space telescope (contrasting with the near- to mid-infrared James Webb Space Telescope) with a large gain in sensitivity over the Herschel Space Observatory (a previous far-infrared telescope), and better angular resolution with at least a four-order of magnitude ...

  7. Interstellar medium - Wikipedia

    en.wikipedia.org/wiki/Interstellar_medium

    The interstellar medium (ISM) is the matter and radiation that exists in the space between the star systems in a galaxy. This matter includes gas in ionic, atomic, and molecular form, as well as dust and cosmic rays. It fills interstellar space and blends smoothly into the surrounding intergalactic space.

  8. Dust astronomy - Wikipedia

    en.wikipedia.org/wiki/Dust_astronomy

    In the low-density (H atoms per ) diffuse interstellar medium, dust particles up to micron size couple with gas clouds within a frictional scale of less than 1 pc. Within the denser, colder interstellar medium found in molecular clouds ( n H = 10 8 − 10 12 m − 3 {\displaystyle {10^{8}-10^{12}m^{-3}}} ), the growth of grains occurs through ...

  9. Tyche (hypothetical planet) - Wikipedia

    en.wikipedia.org/wiki/Tyche_(hypothetical_planet)

    An artist's rendering of the Oort cloud and the Kuiper belt (inset). Tyche / ˈ t aɪ k i / was a hypothetical gas giant located in the Solar System's Oort cloud, first proposed in 1999 by astrophysicists John Matese, Patrick Whitman and Daniel Whitmire of the University of Louisiana at Lafayette.