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  2. Solar radius - Wikipedia

    en.wikipedia.org/wiki/Solar_radius

    6.957 00 × 10 8: metres: 695,700: kilometres: 0.00465047: ... Solar radius is a unit of distance used to express the size of stars in astronomy relative to the Sun.

  3. Sun - Wikipedia

    en.wikipedia.org/wiki/Sun

    The Sun, taking along the whole Solar System, orbits the galaxy's center of mass at an average speed of 230 km/s (828,000 km/h) or 143 mi/s (514,000 mph), [168] taking about 220–250 million Earth years to complete a revolution (a Galactic year), [169] having done so about 20 times since the Sun's formation.

  4. Galactic year - Wikipedia

    en.wikipedia.org/wiki/Galactic_year

    The Solar System is traveling at an average speed of 230 km/s (828,000 km/h) or 143 mi/s (514,000 mph) within its trajectory around the Galactic Center, [3] a speed at which an object could circumnavigate the Earth's equator in 2 minutes and 54 seconds; that speed corresponds to approximately 1/1300 of the speed of light.

  5. Proper motion - Wikipedia

    en.wikipedia.org/wiki/Proper_motion

    This motion is caused by the movement of the stars relative to the Sun and Solar System. The Sun travels in a nearly circular orbit (the solar circle ) about the center of the galaxy at a speed of about 220 km/s at a radius of 8,000 parsecs (26,000 ly) from Sagittarius A* [ 5 ] [ 6 ] which can be taken as the rate of rotation of the Milky Way ...

  6. Peculiar velocity - Wikipedia

    en.wikipedia.org/wiki/Peculiar_velocity

    In galactic astronomy, peculiar motion refers to the motion of an object (usually a star) relative to a Galactic rest frame. Local objects are commonly examined as to their vectors of position angle and radial velocity. These can be combined through vector addition to state the object's motion relative to the Sun.

  7. Milky Way - Wikipedia

    en.wikipedia.org/wiki/Milky_Way

    The Milky Way is approximately 890 billion to 1.54 trillion times the mass of the Sun in total (8.9 × 10 11 to 1.54 × 10 12 solar masses), [7] [8] [9] although stars and planets make up only a small part of this. Estimates of the mass of the Milky Way vary, depending upon the method and data used.

  8. Stellar kinematics - Wikipedia

    en.wikipedia.org/wiki/Stellar_kinematics

    For the Milky Way, the speed of disk stars is = and an RMS (Root mean square) velocity relative to this speed of = . For bulge population stars, the velocities are randomly oriented with a larger relative RMS velocity of V R M S = 150 k m s − 1 {\displaystyle \mathrm {V_{RMS}} =150~\mathrm {km} ~\mathrm {s} ^{-1}} and no net circular velocity ...

  9. Solar System - Wikipedia

    en.wikipedia.org/wiki/Solar_System

    The largest such scale model, the Sweden Solar System, uses the 110-meter (361-foot) Avicii Arena in Stockholm as its substitute Sun, and, following the scale, Jupiter is a 7.5-meter (25-foot) sphere at Stockholm Arlanda Airport, 40 km (25 mi) away, whereas the farthest current object, Sedna, is a 10 cm (4 in) sphere in Luleå, 912 km (567 mi ...