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  2. Position of the Sun - Wikipedia

    en.wikipedia.org/wiki/Position_of_the_Sun

    The Sun appears to move northward during the northern spring, crossing the celestial equator on the March equinox. Its declination reaches a maximum equal to the angle of Earth's axial tilt (23.44° or 23°26') [ 8 ] [ 9 ] on the June solstice , then decreases until reaching its minimum (−23.44° or -23°26') on the December solstice , when ...

  3. Sun path - Wikipedia

    en.wikipedia.org/wiki/Sun_path

    Solstice day arcs as viewed from 70° latitude. At local noon the winter Sun culminates at −3.44°, and the summer Sun at 43.44°. Said another way, during the winter the Sun does not rise above the horizon, it is the polar night. There will be still a strong twilight though. At local midnight the summer Sun culminates at 3.44°.

  4. Sun - Wikipedia

    en.wikipedia.org/wiki/Sun

    The coolest layer of the Sun is a temperature minimum region extending to about 500 km above the photosphere, and has a temperature of about 4,100 K. [77] This part of the Sun is cool enough to allow for the existence of simple molecules such as carbon monoxide and water. [ 81 ]

  5. Earth's rotation - Wikipedia

    en.wikipedia.org/wiki/Earth's_rotation

    At time 1, the Sun and a certain distant star are both overhead. At time 2, the planet has rotated 360 degrees and the distant star is overhead again but the Sun is not (1→2 = one stellar day). It is not until a little later, at time 3, that the Sun is overhead again (1→3 = one solar day).

  6. Newly-released photos capture the sun in highest resolution ...

    www.aol.com/newly-released-photos-capture-sun...

    A velocity map shows the speed and direction that material at the sun's surface is moving. Blue shows movement toward the Solar Orbiter, while red indicates movement away from the spacecraft.

  7. Ecliptic - Wikipedia

    en.wikipedia.org/wiki/Ecliptic

    The ecliptic is the apparent path of the Sun throughout the course of a year. [4] Because Earth takes one year to orbit the Sun, the apparent position of the Sun takes one year to make a complete circuit of the ecliptic. With slightly more than 365 days in one year, the Sun moves a little less than 1° eastward [5] every day.

  8. Analemma - Wikipedia

    en.wikipedia.org/wiki/Analemma

    The east–west component results from the nonuniform rate of change of the Sun's right ascension, governed by the combined effects of Earth's axial tilt and its orbital eccentricity. [ 1 ] One can photograph an analemma by keeping a camera at a fixed location and orientation and taking multiple exposures throughout the year, always at the same ...

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