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  2. Rutherford scattering experiments - Wikipedia

    en.wikipedia.org/wiki/Rutherford_scattering...

    and an impact parameter b equal to the radius of a gold nucleus, 7 × 10 −15 m, the estimated deflection angle θ will be 2.56 radians (147°). If b equals the radius of a gold atom ( 1.44 × 10 −10 m ), the estimated angle is a tiny 0.0003 radians (0.02°).

  3. HR 8799 - Wikipedia

    en.wikipedia.org/wiki/HR_8799

    It is one of the most massive disks known around any star within 300 light years of Earth, and there is room in the inner system for terrestrial planets. [23] There is an additional debris disk just inside the orbit of the innermost planet. [8] The orbital radii of planets e, d, c, and b are 2–3 times those of Jupiter, Saturn, Uranus, and ...

  4. Co-orbital configuration - Wikipedia

    en.wikipedia.org/wiki/Co-orbital_configuration

    The possibility of a trojan planet to Kepler-91b was studied but the conclusion was that the transit-signal was a false-positive. [4] In April 2023, a group of amateur astronomers reported two new exoplanet candidates co-orbiting , in a horseshoe exchange orbit, close to the star GJ 3470 (this star has been known to have a confirmed planet GJ ...

  5. HR 8799 d - Wikipedia

    en.wikipedia.org/wiki/HR_8799_d

    HR 8799 d is an extrasolar planet located approximately 129 light-years away in the constellation of Pegasus, orbiting the 6th magnitude Lambda Boötis star HR 8799.It has a mass between 5 and 10 Jupiter masses and a radius from 20 to 30% larger than Jupiter's.

  6. Newton's theorem of revolving orbits - Wikipedia

    en.wikipedia.org/wiki/Newton's_theorem_of...

    The blue planet feels only an inverse-square force and moves on an ellipse (k = 1). The green planet moves angularly three times as fast as the blue planet (k = 3); it completes three orbits for every orbit of the blue planet. The red planet illustrates purely radial motion with no angular motion (k = 0).

  7. Orbital period - Wikipedia

    en.wikipedia.org/wiki/Orbital_period

    The orbital period (also revolution period) is the amount of time a given astronomical object takes to complete one orbit around another object. In astronomy, it usually applies to planets or asteroids orbiting the Sun, moons orbiting planets, exoplanets orbiting other stars, or binary stars.

  8. Here Are The All-Time Record Cold Low Temperatures In All 50 ...

    www.aol.com/heres-time-record-cold-low-170000238...

    Alaska holds the all-time U.S. record. The mercury plummeted to 80 degrees below zero on Jan. 23, 1971, in Prospect Creek, north of Fairbanks.

  9. List of multiplanetary systems - Wikipedia

    en.wikipedia.org/wiki/List_of_multiplanetary_systems

    One of the oldest stars with a multiplanetary system, although it is still more metal-rich than the Sun. None of the known planets is in the habitable zone. [30] 61 Virginis: Virgo: 13 h 18 m 24.31 s: −18° 18′ 40.3″ 4.74: 28: G5V: 0.954: 5531: 8.96: 2 (1) Planet d remains unconfirmed, [31] and a 2021 study found that it was likely a ...