How to calculate the cycle of solar eclipse on Mars in 2020?

The last solar eclipse on Mars was on July 27th, 20 18. What will the coming Mars bring to the sun? How to calculate the solar cycle of Mars? Then, when it is revealed, the knowledge of the constellation will reveal the date when Mars will hit the sun in 2020. How to calculate the cycle?

When will Mars hit the sun in 2020?

10 On June 14, Mars rushed to the sun.

The timetable for Mars to rush to the sun

2065438+July 27th, 2008 05: 12 0.3862-25 29' Dachong.

202065438+1October 65438+April 23rd: 25 0.4 192+05 26'.

65438+February 8, 2022 05: 4 1 0.5496+24 59'.

065438+ 10 June 65438+June 2025 02: 38 0.6437+25 06'.

February 20271915: 50 0.6779+1522' Xiaochong.

March 25th, 2029 07: 48 0.6495438+0+0 1 04'.

203 1 05 04 12:03 0.5589- 15 28 '。

June 28th, 2033 0 1: 29 0.4272-27 49'.

September 20351519: 38 0.817-0802' Dachong.

2037 165438+ 10/9 09 0.4996+2016'.

0 12 2040 10 month15: 26 0.6136+26 41'.

How to calculate the solar cycle of Mars?

There is an eclipse every 779 and 782 days. Eclipses do not occur every eclipse, but only in individual eclipses. Eclipses on Mars occur regularly, about 8 times every 17 years, that is, about every 2 years 1 times.

The rendezvous period of other planets

Jupiter: 398.88 days.

Saturn: 378.09 days.

What is Mars rushing to the sun?

Mars rushing to the sun means that Mars, the earth and the sun are almost in a line, and the earth is located between the sun and Mars. At this time, the side of Mars illuminated by the sun is completely facing the earth, so it is bright and easy to observe. The interval between two adjacent solar eclipses on Mars is about 779 days, and the last one appeared on 2065438+July 27, 2008. The next eclipse of Mars will occur in June 65438 +654381October+April 2020.

Because the surface activity (such as surface sandstorm) or surface topography of Mars at perihelion can be seen with naked eyes, Mars is under the importance of human exploration of extraterrestrial civilization, and the apparent diameter of Mars rushing to the sun will be much larger than at other times, so that the surface condition can be clearly seen. Therefore, many astronomy enthusiasts or observatories will take part in the observation and record the changes of Martian dust storms and polar caps, mostly during the eclipse of Mars.