Tiina Hölli: (Untitled)

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on
autumnal equinox
September 23rd 2015

Syyspäiväntasaus on hetki,
jolloin Aurinko ohittaa taivaan ekvaattorin
ja on suoraan päiväntasaajan yläpuolella.

Sekä kevät- että syyspäiväntasauksessa
aika auringonnoususta auringonlaskuun
on 12 tuntia koko maapallolla.

Vuonna 2015 syyspäiväntasaus on 23. syyskuuta.
Täsmällinen hetki on 11.21 Suomen aikaa.

Talvipäivänseisaus on 22.12. kello 06.48.

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Who, What, Why: What is an equinox?
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The answer

One of the two days of the year where everywhere in the world
theoretically experiences the same length of day and night.
This is prevented during the rest of the year by the tilt of the earth

quoting

BBC News Magazine´s email Newsletter 23 September 2015

http://www.bbc.co.uk/news/magazine-34334712?ns_mchannel=email&ns_source=inxmail_newsletter&ns_campaign=bbcnewsmagazine_news__&ns_linkname=na&ns_fee=0

The name equinox means "equal night" in Latin. It's theoretically the day of the year when all points on the earth's surface experience the same lengths of daylight and darkness - 12 hours of each. The autumn equinox in the northern hemisphere (it's the spring equinox for the southern hemisphere) always falls on 22, 23 or 24 September.

Imagine the earth orbiting the sun in a flat plane - ie as if it was pinned on the edge of a slightly elliptical disc. It spins on its axis as it does so - each turn making a day. But the earth also constantly tilts at an angle of 23.5 degrees to that flat plane as it orbits the sun.

This means, for half the year, the northern hemisphere is pointing slightly away from the sun, bringing shorter, colder days as it moves into winter. For the other half of the year it points slightly towards the sun, getting longer, hotter days, most extreme in high summer.

But the equinoxes (there's one in March, too) are the points of the year where the part of the earth closest to the sun is the equator rather than places north or south of it. Everywhere from the North Pole to the South Pole gets the same number of hours of sunlight, just for those two days a year.

In theory everywhere on earth should get half a day of sun and half a day of darkness when an equinox happens. "But this is complicated by the fact that the earth has an atmosphere," says Robert Massey, deputy executive director of the Royal Astronomical Society. "This means when the sun's near the horizon it appears to be slightly higher than it is because the light is refracted through the atmosphere. So, you get slightly longer than the 12 hours of sunlight."

If the earth didn't tilt, every day would be an equinox, as the sun would always be closest to the equator. There would not be winters or summers as we know them, says Massey.

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