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  2. List of hottest exoplanets - Wikipedia

    en.wikipedia.org/wiki/List_of_hottest_exoplanets

    This is a list of the hottest exoplanets so far discovered, specifically those with temperatures greater than 2,500 K (2,230 °C; 4,040 °F) for exoplanets irradiated by a nearby star and greater than 2,000 K (1,730 °C; 3,140 °F) for self-luminous exoplanets.

  3. Plasma (physics) - Wikipedia

    en.wikipedia.org/wiki/Plasma_(physics)

    [16] [17] [18] It is a state of matter in which an ionized substance becomes highly electrically conductive to the point that long-range electric and magnetic fields dominate its behaviour. [19] [20] Plasma is typically an electrically quasineutral medium of unbound positive and negative particles (i.e., the overall charge of a plasma is ...

  4. Helium - Wikipedia

    en.wikipedia.org/wiki/Helium

    All heavier elements (including those necessary for rocky planets like the Earth, and for carbon-based or other life) have thus been created since the Big Bang in stars which were hot enough to fuse helium itself. All elements other than hydrogen and helium today account for only 2% of the mass of atomic matter in the universe.

  5. Gas giant - Wikipedia

    en.wikipedia.org/wiki/Gas_giant

    The term gas giant was coined in 1952 by the science fiction writer James Blish [6] and was originally used to refer to all giant planets.It is, arguably, something of a misnomer because throughout most of the volume of all giant planets, the pressure is so high that matter is not in gaseous form. [7]

  6. List of hottest stars - Wikipedia

    en.wikipedia.org/wiki/List_of_hottest_stars

    This is a list of hottest stars so far discovered (excluding degenerate stars), arranged by decreasing temperature. The stars with temperatures higher than 60,000 K are included. List

  7. Orders of magnitude (temperature) - Wikipedia

    en.wikipedia.org/wiki/Orders_of_magnitude...

    Particular speeds bound paths to exceed the size and lifetime of the universe, i.e. the particle's total path traveled (but not the distance from its place of origin) since the beginning of the universe is less than the size of the universe [further explanation needed] (see least-energy in orders of magnitude (energy))

  8. Quark–gluon plasma - Wikipedia

    en.wikipedia.org/wiki/Quark–gluon_plasma

    The new phase of matter, consisting of dissolved hadrons, exhibits less resistance to flow than any other known substance. The experiments at RHIC have, already in 2005, shown that the Universe at its beginning was uniformly filled with this type of material—a super-liquid—which once the Universe cooled below T H evaporated into a gas of ...

  9. R136a1 - Wikipedia

    en.wikipedia.org/wiki/R136a1

    R136a1 (short for RMC 136a1) is one of the most massive and luminous stars known, at nearly 200 M ☉ and nearly 4.7 million L ☉, and is also one of the hottest, at around 46,000 K. It is a Wolf–Rayet star at the center of R136 , the central concentration of stars of the large NGC 2070 open cluster in the Tarantula Nebula (30 Doradus ) in ...