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  2. File:Kepler-9b, Jupiter size comparison.jpg - Wikipedia

    en.wikipedia.org/wiki/File:Kepler-9b,_Jupiter...

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  3. Jupiter - Wikipedia

    en.wikipedia.org/wiki/Jupiter

    Based on Jupiter's composition, researchers have made the case for an initial formation outside the molecular nitrogen (N 2) snow line, which is estimated at 20–30 AU (3.0–4.5 billion km; 1.9–2.8 billion mi) from the Sun, and possibly even outside the argon snow line, which may be as far as 40 AU (6.0 billion km; 3.7 billion mi).

  4. Rings of Jupiter - Wikipedia

    en.wikipedia.org/wiki/Rings_of_Jupiter

    Its outer edge is located at a radius of about 129,000 km (1.806 R J;R J = equatorial radius of Jupiter or 71,398 km) and coincides with the orbit of Jupiter's smallest inner satellite, Adrastea. [ 2 ] [ 5 ] Its inner edge is not marked by any satellite and is located at about 122,500 km ( 1.72 R J ).

  5. Bristol Jupiter - Wikipedia

    en.wikipedia.org/wiki/Bristol_Jupiter

    Bristol Jupiter X 470 hp (350 kW); compression ratio 5.3:1. Bristol Jupiter XF 540 hp (400 kW); version of Jupiter X with forged cylinder heads Bristol Jupiter XFA 483 hp (360 kW) Bristol Jupiter XFAM 580 hp (430 kW) Bristol Jupiter XFBM 580 hp (430 kW) Bristol Jupiter XFS Fully supercharged. Bristol Jupiter XI Compression ratio 5.15:1.

  6. Carme group - Wikipedia

    en.wikipedia.org/wiki/Carme_group

    The parent body was probably about the size of Carme, 46 km in diameter; 99% of the group's mass is still located in Carme. [ 6 ] Further support to the single body origin comes from the known colours: all the satellites appear light red, [ c ] with colour indices B-V= 0.76 and V-R= 0.47 [ 7 ] and infrared spectra , similar to D-type asteroids ...

  7. Schmidt coupling - Wikipedia

    en.wikipedia.org/wiki/Schmidt_coupling

    A Schmidt coupling is a type of coupling designed to accommodate large radial displacement between two shafts. Consisting of an arrangement of links and discs—three discs rotating in unison, interconnected in series by three or more links between each pair of discs—a Schmidt coupling can adapt to very wide variations in radial displacement while running under load.

  8. Jupiter radius - Wikipedia

    en.wikipedia.org/wiki/Jupiter_radius

    The Jupiter radius or Jovian radius (R J or R Jup) has a value of 71,492 km (44,423 mi), or 11.2 Earth radii (R 🜨) [2] (one Earth radius equals 0.08921 R J). The Jupiter radius is a unit of length used in astronomy to describe the radii of gas giants and some exoplanets. It is also used in describing brown dwarfs.

  9. Tempel 1 - Wikipedia

    en.wikipedia.org/wiki/Tempel_1

    Tempel 1 (official designation: 9P/Tempel) is a periodic Jupiter-family comet discovered by Wilhelm Tempel in 1867. It completes an orbit of the Sun every 5.6 years. Tempel 1 was the target of the Deep Impact space mission, which photographed a deliberate high-speed impact upon the comet in 2005.

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