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"Freed from Desire" is a Eurodance song by Italian singer and songwriter Gala. Produced by DJ Molella and Phil Jay it was released in 1996 as the first single from her debut album, Come into My Life (1997). It was a hit in many European countries, reaching number one in France and Belgium (Flanders and Wallonia). The track was released in the ...
"Desire" is a song by Scottish DJ and record producer Calvin Harris and English singer and songwriter Sam Smith. It was released on 28 July 2023 through Columbia Records and Sony Music UK and included on Harris' first compilation album , 96 Months (2024).
Mars's average distance from the Sun is roughly 230 million km (143 million mi), and its orbital period is 687 (Earth) days. The solar day (or sol) on Mars is only slightly longer than an Earth day: 24 hours, 39 minutes, and 35.244 seconds. [185] A Martian year is equal to 1.8809 Earth years, or 1 year, 320 days, and 18.2 hours. [2]
As if that isn’t cool enough, you can also see 100% of Mars’ disk lit up by the sun that night—AKA the entire face of Mars will be visible. Related: How to Organize Your Weekly Schedule ...
The average duration of the day-night cycle on Mars — i.e., a Martian day — is 24 hours, 39 minutes and 35.244 seconds, [3] equivalent to 1.02749125 Earth days. [4] The sidereal rotational period of Mars—its rotation compared to the fixed stars—is 24 hours, 37 minutes and 22.66 seconds. [4]
The length of time for Mars to complete one orbit around the Sun in respect to the stars, its sidereal year, is about 686.98 Earth solar days (≈ 1.88 Earth years), or 668.5991 sols. Because of the eccentricity of Mars' orbit, the seasons are not of equal length.
Extra-close oppositions of Mars happen every 15 to 17 years, when we pass between Mars and the Sun around the time of its perihelion (closest point to the Sun in orbit). The minimum distance between Earth and Mars has been declining over the years, and in 2003 the minimum distance was 55.76 million km, nearer than any such encounter in almost ...
Solar longitude, commonly abbreviated as Ls, is the ecliptic longitude of the Sun, i.e. the position of the Sun on the celestial sphere along the ecliptic.It is also an effective measure of the position of the Earth (or any other Sun-orbiting body) in its orbit around the Sun, [1] usually taken as zero at the moment of the vernal equinox. [2]