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  2. Solar wind - Wikipedia

    en.wikipedia.org/wiki/Solar_wind

    The total number of particles carried away from the Sun by the solar wind is about 1.3 × 10 36 per second. [32] Thus, the total mass loss each year is about (2–3) × 10 −14 solar masses, [33] or about 1.3–1.9 million tonnes per second. This is equivalent to losing a mass equal to the Earth every 150 million years. [34]

  3. Solar activity and climate - Wikipedia

    en.wikipedia.org/wiki/Solar_activity_and_climate

    [28] [42] Lockwood and Fröhlich, 2007, found "considerable evidence for solar influence on the Earth's pre-industrial climate and the Sun may well have been a factor in post-industrial climate change in the first half of the last century", but that "over the past 20 years, all the trends in the Sun that could have had an influence on the Earth ...

  4. Milankovitch cycles - Wikipedia

    en.wikipedia.org/wiki/Milankovitch_cycles

    [46] Another work [47] suggests that solar insolation at 65° N will reach a peak of 460 W·m −2 in around 6,500 years, before decreasing back to current levels (450 W·m −2) [48] in around 16,000 years. Earth's orbit will become less eccentric for about the next 100,000 years, so changes in this insolation will be dominated by changes in ...

  5. Michelson–Morley experiment - Wikipedia

    en.wikipedia.org/wiki/Michelson–Morley_experiment

    In the table below, the expected values are related to the relative speed between Earth and Sun of 30 km/s (18.6 mi/s). With respect to the speed of the solar system around the galactic center of about 220 km/s (140 mi/s), or the speed of the solar system relative to the CMB rest frame of about 370 km/s (230 mi/s), the null results of those ...

  6. List of solar cycles - Wikipedia

    en.wikipedia.org/wiki/List_of_solar_cycles

    Solar cycles are nearly periodic 11-year changes in the Sun's activity that are based on the number of sunspots present on the Sun's surface. The first solar cycle conventionally is said to have started in 1755.

  7. Solar cycle - Wikipedia

    en.wikipedia.org/wiki/Solar_cycle

    In 1974 the book The Jupiter Effect suggested that the alignment of the planets would alter the Sun's solar wind and, in turn, Earth's weather, culminating in multiple catastrophes on March 10, 1982. None of the catastrophes occurred.

  8. Solar phenomena - Wikipedia

    en.wikipedia.org/wiki/Solar_phenomena

    The Earth's mean distance from the Sun is approximately 1 astronomical unit (about 150,000,000 km; 93,000,000 mi), though the distance varies as the Earth moves from perihelion in January to aphelion in July. [12] At this average distance, light travels from the Sun to Earth in about 8

  9. 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), [167] taking about 220–250 million Earth years to complete a revolution (a Galactic year), [168] having done so about 20 times since the Sun's formation.