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  1. at the surface of the Sun is about 55. 0oC (5800 K). Just like the Earth, the Sun rotates. However, unlike the Earth, the Sun is not a solid body, this means that the gas that forms its surface does not move as one p.

  2. Jul 26, 2022 · To this day, astronomers and solar scientists use sunspots and other features on the surface of our star to measure its rotation. Yet, there is more to learn about the sun's rotation....

  3. nssdc.gsfc.nasa.gov › planetary › factsheetSun Fact Sheet - NSSDCA

    Rotational and Orbital parameters. *This is the adopted period at 16 deg. latitude - the actual rotation rate varies with latitude L as: ( 14.37 - 2.33 sin 2 L - 1.56 sin 4 L ) deg/day. North Pole of Rotation. Right Ascension: 286.13 Declination : 63.87 Reference Date : 1.5 Jan 2000 (JD 2451545.0) Sun Observational Parameters.

  4. Measuring a “day” on the Sun is complicated. The Sun is made of super-hot, electrically charged gas called plasma. This plasma rotates at different speeds on different parts of the Sun. At its equator, the Sun completes one rotation in 25 Earth days. At its poles, the Sun rotates once on its axis every 36 Earth days.

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  5. en.wikipedia.org › wiki › SunSun - Wikipedia

    At great distances, the rotation of the Sun twists the dipolar magnetic field and corresponding current sheet into an Archimedean spiral structure called the Parker spiral. [85]

  6. sun on June 10 gives a distorted linear measure due to foreshortening. The sun has rotated about 20 degrees during the 2 days, so that means a full rotation would take about (365/20) x 2 days = 36.5 days which is closer to the equatorial speed of the sun of 35 days.

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  8. Mar 2, 2016 · To determine the Sun’s rotational period using images of a sunspot from the SOHO database, each group should measure the displacement (x) – the distance of their sunspot from the central axis of the Sun – at a succession of times (t) with a ruler.

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