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  1. 4 lip 2010 · In order to keep the sun in the same position in the sky by flying due west you need a speed of 1035 mph times cosine(latitude). That means it takes the full 1035 mph at equator and only half, around 500 mph, at 60 deg north or south (cos(60) = 0.5).

  2. 13 wrz 2009 · The speed of sound at sea level is about 800 miles an hour. So, to keep the sunset in view – as seen from the latitude of the equator – you’d have to drive your car fast enough to break...

  3. Mach Speed is when an object moves faster than the speed of sound. For normal and dry conditions and temperature of 68 degrees F, this is 768 mph, 343 m/s, 1,125 ft/s, 667 knots, or 1,235 km/h.

  4. 29 kwi 2016 · Sharpening its point, the H1 quickly set acceleration records, with Tony Nicosia making a quarter-mile run of 12.96 seconds at 100.7 miles per hour aboard the raging triple.

  5. 10 gru 2015 · At the North Pole, the sun starts setting at 24 Sep 2015 at 0243, and finishes setting at 25 Sep 2015 at 1131, a length of 32 hours and 48 minutes. Main caveat: Like HORIZONS and the sunrise/sunset tables above, I assume 34 arcminutes of refraction at the horizon.

  6. 4 lis 2020 · From 35° S latitude (latitude = -35), the winter Sun would rise at $\theta=119$ from due south (or 61° from due north, approximately ENE). The summer Sun would rise at $\theta=61$ from due south (or 119° from due north, approximately ESE). The range is 119-61=58° along the horizon.

  7. 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.

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