The June 2014 Solstice

During the solstices, Earth reaches a point where its tilt is at the greatest angle to the plane of its orbit, causing one hemisphere to receive more daylight than the other. (NASA/Genna Duberstein)

During the solstices, Earth reaches a point where its tilt is at the greatest angle to the plane of its orbit, causing one hemisphere to receive more daylight than the other. (NASA/Genna Duberstein)

The June solstice for 2014 begins on June 21st at 10:51 UT (6:51 am EDT.) It is called the summer solstice for the Northern Hemisphere and the winter solstice for the Southern Hemisphere.

During the solstices, Earth reaches a point where its tilt is at the greatest angle to the plane of its orbit, causing one hemisphere to receive more daylight than the other. (NASA/Genna Duberstein)

During the solstices, Earth reaches a point where its tilt is at the greatest angle to the plane of its orbit, causing one hemisphere to receive more daylight than the other. (NASA/Genna Duberstein)

But what is the solstice exactly?

There are two solstices in a year, the June solstice (usually June 21) and the December solstice (usually December 21). On the June solstice the sun reaches its highest point in the sky for an observer at the North Pole. On the December solstice the sun reaches its highest point in the sky for an observer at the South Pole. Solstices also mark the change from fall to winter or spring to summer.

The solstices happen because of the tilt of Earth’s axis of rotation with respect to its orbital path around the sun. The axis of rotation is an imaginary line drawn straight through Earth connecting the North Pole to the South Pole. This line is tilted 23.5° from Earth’s orbital path around the Sun. This means that the sun’s light does not hit the Earth evenly at a particular latitude above and below the equator. This tilt is the cause of Earth’s seasons. (The equator is an imaginary line drawn right around Earth’s middle, like a belt. It divides Earth into the Northern  and the Southern Hemispheres. The imaginary lines around Earth that are parallel to the Equator are called lines of latitude. They are numbered from 0° to 90°. The one at 0° is the equator itself. The higher the number, the farther north (if it’s a + number) or south (if it’s a − number). )

Because of Earth’s tilt is 23.5° the latitudes of +23.5° and −23.5° are special and have special names. The one in the Northern Hemisphere,  +23.5° latitude, is called the Tropic of Cancer. The one in the Southern Hemisphere, − 23.5° latitude, is called the Tropic of Capricorn.

These are the latitudes where the Sun is directly overhead at noon once a year. In the Northern hemisphere, on the Tropic of Cancer, that is the June Solstice. In the Southern Hemisphere, on the Tropic of Capricorn, that is the December Solstice. These solstice days are the days with the most (for Summer) or fewest (for Winter) hours of sunlight during the whole year.

For the northern hemisphere, the Sun is directly overhead at "high-noon" on Summer Solstice at the latitude called the Tropic of Cancer.

For the northern hemisphere, the Sun is directly overhead at “high-noon” on Summer Solstice at the latitude called the Tropic of Cancer.

Every six months, Jan Koeman of Zierikzee, the Netherlands, uses a beer-can solargraph to record the progress of the sun in the sky from solstice to solstice. This year he placed his solargraph inside a lighthouse but he was worried if the lighthouse would overpower the solargraph so he opened it one week early.

Click on an image below to view larger.

Koeman explained, “Just one week to go before the summer solstice. Time to check your solarcans if they are still there after 6 months exposuretime. I can’t wait until next week and wanted to know if the light in a lighthouse is overexposing the sunlight. I did put a solarcan inside the lighthouse. Luckily our sun is much stronger. The fresnel prisms in the lighthouse were chopping up the sunlight.”

 credit: NASA/spaceweather.com/Jan Koeman