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  2. Nebular hypothesis - Wikipedia

    en.wikipedia.org/wiki/Nebular_hypothesis

    The nebular hypothesis is the most widely accepted model in the field of cosmogony to explain the formation and evolution of the Solar System (as well as other planetary systems ). It suggests the Solar System is formed from gas and dust orbiting the Sun which clumped up together to form the planets. The theory was developed by Immanuel Kant ...

  3. List of Solar System objects by size - Wikipedia

    en.wikipedia.org/wiki/List_of_Solar_System...

    Relative masses of the Solar planets. Jupiter at 71% of the total and Saturn at 21% dominate the system. Relative masses of the solid bodies of the Solar System. Earth at 48% and Venus at 39% dominate. Bodies less massive than Pluto are not visible at this scale. Relative masses of the rounded moons of the Solar System.

  4. Solar System model - Wikipedia

    en.wikipedia.org/wiki/Solar_System_model

    The Boston Museum of Science had placed bronze models of the planets in major public buildings, all on similar stands with interpretive labels. [1] For example, the model of Jupiter was located in the cavernous South Station waiting area. The properly-scaled, basket-ball-sized model is 1.3 miles (2.14 km) from the model Sun which is located at ...

  5. Titius–Bode law - Wikipedia

    en.wikipedia.org/wiki/Titius–Bode_law

    Subsequent research detected 5 candidate planets from the 97 planets predicted for the 68 planetary systems. The study showed that the actual number of planets could be larger. The occurrence rates of Mars- and Mercury-sized planets are currently unknown, so many planets could be missed due to their small size.

  6. Orrery - Wikipedia

    en.wikipedia.org/wiki/Orrery

    Orrery. An orrery is a mechanical model of the Solar System that illustrates or predicts the relative positions and motions of the planets and moons, usually according to the heliocentric model. It may also represent the relative sizes of these bodies; however, since accurate scaling is often not practical due to the actual large ratio ...

  7. Geocentric model - Wikipedia

    en.wikipedia.org/wiki/Geocentric_model

    Most noticeably the size of a planet's retrograde loop (especially that of Mars) would be smaller, or sometimes larger, than expected, resulting in positional errors of as much as 30 degrees. To alleviate the problem, Ptolemy developed the equant. The equant was a point near the center of a planet's orbit where, if you were to stand there and ...

  8. NASA finds evidence of 10 new Earth-size planets that could ...

    www.aol.com/article/news/2017/06/20/nasa-finds...

    NASA just announced that they've found 219 potential planets, and of those, 10 are close to the size of Earth and could possibly sustain life.

  9. Template:Planetary radius - Wikipedia

    en.wikipedia.org/wiki/Template:Planetary_radius

    Directory. This template is to show size comparison of Jupiter, Neptune and the Earth alongside extrasolar planets that have their radial size confirmed. {{Planetary radius | radius = <!--simplified number of the radius (Jupiter equals 100px)--> }} Some planets might have a radius that would be hard to compare to Jupiter.