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  1. On the top text field you can visualize the distance value from default to the last point, measured in Km, mile (mi) or for short distance meters (m), foot (ft). This is very useful to calculate the distance of a path of trekking, mountain bike, sport, free time ...

    • Sun Position

      Sun chart Sun path charts can be plotted either in Cartesian...

    • Coordinates Conversion

      Format Value range Valid value for the latitude are from...

    • Print

      | SunEarthTools.com | Tools for consumers and designers of...

    • Info

      year: month: day: hour: minute ...

  2. SunCalc shows the movement of the sun and sunlight-phase for a certain day at a certain place. You can change the suns positions for sunrise, selected time and sunset see. The thin yellow-colored curve shows the trajectory of the sun, the yellow deposit shows the variation of the path of the sun throughout the year.

  3. Shadow calculator, sun position, sun path and sun exposure. Simulate shadows cast by buildings, trees and terrain in 3D. Sunlight and shading for sunrise and sunset photos. Prepare a shadow study, shadow analysis or solar analysis. No need to install or buy Google Earth Pro. Works online.

  4. Solar position calculator. Location: Latitude: Longitude: This chart shows the path of the Sun in the sky today, during the summer solstice and the winter solstice based on the location you enter in the search bar. The red dot represents the current apparent position of the Sun in terms of azimuth and elevation.

  5. 16 kwi 2019 · Calculating Noon Sun Angles. First, find the distance in degrees between . the latitude of where you are and where the Sun’s most direct rays are shining on Earth at that time of year. Then subtract that number from 90°. The most direct rays of the Sun are shining at: • 23.5°N on the summer solstice • 0° (the equator) on the equinoxes

  6. A little online application with interactive map that shows sun movement and sunlight phases during the given day at the given location.

  7. 15 lut 2011 · From this, they deduced the distance Earth-Mars. Then, using the Kepler law $$\frac{a^3}{p^2}= constant$$ (where $a$ is the distance between the planet and the Sun, and $p$ the sideral time) they could figure out what was the distance to the Sun.

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