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  2. Supernova - Wikipedia

    en.wikipedia.org/wiki/Supernova

    The surrounding material is blasted away (f), leaving only a degenerate remnant. [109] When a stellar core is no longer supported against gravity, it collapses in on itself with velocities reaching 70,000 km/s (0.23c), [110] resulting in a rapid increase in temperature and density. What follows depends on the mass and structure of the ...

  3. (471325) 2011 KT19 - Wikipedia

    en.wikipedia.org/wiki/(471325)_2011_KT19

    Light-curve analysis from 2016 showed only small deviations, which suggested that 2011 KT 19 is a spheroid about 250 km with small albedo spots and hence a dwarf planet. It is not included in Michael E. Brown's number of dwarf planet candidates from now because, having an assumed albedo of 0.08 and an absolute magnitude of 7.4, it would be less ...

  4. TRAPPIST-1f - Wikipedia

    en.wikipedia.org/wiki/TRAPPIST-1f

    TRAPPIST-1f, also designated as 2MASS J23062928-0502285 f, is an exoplanet, likely rocky, [2] orbiting within the habitable zone [5] around the ultracool dwarf star TRAPPIST-1, located 40.7 light-years (12.5 parsecs) away from Earth in the constellation of Aquarius.

  5. Gamma-ray burst - Wikipedia

    en.wikipedia.org/wiki/Gamma-ray_burst

    The Space Variable Objects Monitor is a small X-ray telescope satellite for studying the explosions of massive stars by analysing the resulting gamma-ray bursts, developed by China National Space Administration (CNSA), Chinese Academy of Sciences (CAS) and the French Space Agency , [45] launched on 22 June 2024 (07:00:00 UTC).

  6. Phaeton (hypothetical planet) - Wikipedia

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

    Phaeton (alternatively Phaethon / ˈ f eɪ. ə θ ən / or Phaëton / ˈ f eɪ. ə t ən /; from Ancient Greek: Φαέθων, romanized: Phaéthōn, pronounced [pʰa.é.tʰɔːn]) is a hypothetical planet hypothesized by the Titius–Bode law to have existed between the orbits of Mars and Jupiter, the destruction of which supposedly led to the formation of the asteroid belt (including the ...

  7. Astronomers surprised to find planet 'too massive for its star'

    www.aol.com/news/astronomers-surprised-planet...

    The planet, called LHS 3154 b, orbits at about 2.3% of Earth's orbital distance from the sun, circling its star every 3.7 days. It is much closer even than our solar system's innermost planet ...

  8. Gravitational collapse - Wikipedia

    en.wikipedia.org/wiki/Gravitational_collapse

    Gravitational collapse of a massive star, resulting in a Type II supernova. Gravitational collapse is the contraction of an astronomical object due to the influence of its own gravity, which tends to draw matter inward toward the center of gravity. [1]

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