Mars Year 1
Mars Year 1 is the first year of Martian timekeeping standard developed by Clancy et al. originally for the purposes of working with the cyclical temporal variations of meteorological phenomena of Mars, but later used for general timekeeping on Mars. Mars Years have no officially adopted month systems. Scientists generally use two sub-units of the Mars Year:
- the Solar longitude system: 360 degrees per Mars Year that represent the position of Mars in its orbit around the Sun, or
- the Sol system: 668 sols per Mars Year. This system consists of uniform time units. However, Mars Year sols may be confused with rover mission times that are also expressed in sols.
Mars Year 1 started on 11 April 1955 and ended on 25 February 1957. Mars Year 1 is preceded by Mars Year 0.
Events of Mars Year 1
There was no spacecraft on or around Mars in Mars Year 1.De Mottoni created two albedo maps, Kuiper made several drawings Millman made maps and detailed descriptions and Dollfus observed the poles of Mars during the 1956 opposition.
- Ls 257 Křivský et al. reports that the polar cap disappeared during a solar flare event.
- Ls 263 : Earth is closest to Mars. This was the best time to observe Mars, therefore most observations during M.Y. 1 took place during this time.
- Around Ls 270: Major dust storm. Kuiper observed that a new polar cap formed before the southern summer solstice, and a dust storm developed over Mare Sirenum or Hellespontus and spread rapidly, covering the entire planet with dust except the south polar region. The lowered temperature may have led to the early formation of the polar cap where bright white snow was observed uncontaminated by yellow dust, however Millman attributes the disappearance of the cap to clouds.