June 20th, 2016 marks the official beginning of summer in the northern hemisphere. We call this day the summer solstice.
In astronomical terms, the summer solstice for the northern hemisphere occurs when the sun is the farthest north of the equator on the ecliptic. This angular distance is 23.5°, This angle also marks a line of latitude on the Earth called the Tropic of Cancer.
The Tropic of Cancer is so called because the summer solstice used to occur when the Sun was in the constellation Cancer and the latitude lines in the tropical zone. There is also a comparable line of latitude south of the equator called the Antarctic Circle. The latitude is 66.5° South and for anyone living south of this latitude (really, mostly penguins or anyone stationed in Antarctica), the Sun will never rise. Conversely, the Arctic Circle at 66.5° North, the Sun never sets. In fact, from the vernal equinox to the autumnal equinox, the North Pole is in perpetual sunlight, while the South Pole is in perpetual darkness.
The summer solstice marks the day of the year when the northern hemisphere receives the most light. From here on until the winter solstice, the days will only get shorter and the nights longer. In the southern hemisphere, the opposite occurs. Today marks the shortest day of the year and they are in winter time.
Our universe is filled with strange and wacky things. This blog hopes to point out all the unique things that make the cosmos interesting and fun to learn about.
Showing posts with label equator. Show all posts
Showing posts with label equator. Show all posts
20 June 2016
20 October 2014
The Unusual Inclination of Uranus
Remember way back in June when we talked about the strange inclination of Venus? Believe it or not, there is one planet that has a stranger inclination. Here, the Sun does not rise in the west and set in the east. But then, it doesn't really rise in the east or set in the west all year long. For a portion of its year, Uranus has a hemisphere completely illuminated and another hemisphere completely in the dark.
Uranus inclination is about 98°, which means that its rotational axis is nearly perpendicular to its orbital axis. Another way of saying this, is that Uranus rotates on its side. This means that for a portion of its year, the north pole of Uranus is almost pointed straight at the Sun and the northern hemisphere is almost completely sunlight while the south pole is pointed away from the Sun and therefore, the southern hemisphere is dark. Vice versa, halfway around its orbit, the south pole is pointed towards the Sun and the north pole away.
This phenomena happens on Earth, but not as extreme. There are two latitudes, one north of the equator and one south of the equator, where in the northern summer, at any location north of the northern latitude the Sun will never set and in the northern winter, the Sun will never rise. The same thing happens in the southern latitudes near Antarctica. These latitudes are called the Arctic Circle and the Antarctic Circle. If you have heard of "The Land of the Midnight Sun", this is in reference to the Arctic Circle. On Earth, these circles are at 66.5° North for the Arctic Circle and 66.5° South for the Antarctic Circle. If you recall from science class, that the Earth is tilted 23.5° with respect to the Earth's orbital plane, those two angles equal 90°. On Uranus, it is a little more complicated than that.
When the north pole of Uranus is pointed towards the Sun (or the northern "summer" on Uranus), any latitude north of 8°N will never see the Sun set and any latitude south of 8°S on Uranus will never see the Sun rise. Vice versa, in the southern "summer" on Uranus, any latitude south of 8°S will never see the Sun set and any latitude north of 8°N will never see the Sun rise.
Why does Uranus have such an extreme inclination? Much like Venus, it is believed that soon after formation, Uranus was hit by a large object that knocked it on its side, but because it has a much larger mass than Venus, it did not flip upside down, but rather just onto its side.
Uranus inclination is about 98°, which means that its rotational axis is nearly perpendicular to its orbital axis. Another way of saying this, is that Uranus rotates on its side. This means that for a portion of its year, the north pole of Uranus is almost pointed straight at the Sun and the northern hemisphere is almost completely sunlight while the south pole is pointed away from the Sun and therefore, the southern hemisphere is dark. Vice versa, halfway around its orbit, the south pole is pointed towards the Sun and the north pole away.
This phenomena happens on Earth, but not as extreme. There are two latitudes, one north of the equator and one south of the equator, where in the northern summer, at any location north of the northern latitude the Sun will never set and in the northern winter, the Sun will never rise. The same thing happens in the southern latitudes near Antarctica. These latitudes are called the Arctic Circle and the Antarctic Circle. If you have heard of "The Land of the Midnight Sun", this is in reference to the Arctic Circle. On Earth, these circles are at 66.5° North for the Arctic Circle and 66.5° South for the Antarctic Circle. If you recall from science class, that the Earth is tilted 23.5° with respect to the Earth's orbital plane, those two angles equal 90°. On Uranus, it is a little more complicated than that.
When the north pole of Uranus is pointed towards the Sun (or the northern "summer" on Uranus), any latitude north of 8°N will never see the Sun set and any latitude south of 8°S on Uranus will never see the Sun rise. Vice versa, in the southern "summer" on Uranus, any latitude south of 8°S will never see the Sun set and any latitude north of 8°N will never see the Sun rise.
Why does Uranus have such an extreme inclination? Much like Venus, it is believed that soon after formation, Uranus was hit by a large object that knocked it on its side, but because it has a much larger mass than Venus, it did not flip upside down, but rather just onto its side.
Labels:
Astronomy,
equator,
inclination,
orbit,
poles,
Solar System,
solar year,
Sun,
Uranus
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