Johannes Kepler is an mathematician an astronomer and an astrologerhe also created keplers lawGood, thanks for asking.-Ol' Johannes
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The first note of the major scale is the tonic.
The first note of a major or minor scale is called the tonic note. For example: for C major, the first note (or tonic note) is C; for a minor, the first note (or tonic note) is a.
Major Seventh
Kepler's Third Law, also known as the Harmonic Law, states that the square of the orbital period of a planet is directly proportional to the cube of the semi-major axis of its orbit.
Known for his eponymous laws of planetary motion.
Yes, Kepler's third law applies to all the planets in our solar system. It states that the square of a planet's orbital period is proportional to the cube of its semi-major axis. This relationship holds true for all the planets, with each planet's orbital period and distance from the Sun following this law.
You can find the major axis, 0.5+31.5 or 32 AU. The semimajor axis is half that, 16 AU. Then you can use Keplers 3rd law to calculate the period, which is 161.5 or 64 years.
"The Sugarland Express" (1974).
Johannes Kepler is an mathematician an astronomer and an astrologerhe also created keplers lawGood, thanks for asking.-Ol' Johannes
the 1s orbital is closer to the nucleus and has a lower energy level compared to the 2s orbital. Additionally, the 2s orbital has a slightly higher energy, larger size, and can hold more electrons than the 1s orbital.
For larger orbital radii, the orbital periods increase. This is because the gravitational force decreases with distance, leading to slower speeds and longer times to complete an orbit. Kepler's third law states that the square of the orbital period is proportional to the cube of the semi-major axis length.
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To calculate the orbital period using the semi-major axis, you can use Kepler's third law of planetary motion. The formula is T2 (42 / G(M1 M2)) a3, where T is the orbital period in seconds, G is the gravitational constant, M1 and M2 are the masses of the two objects in the orbit, and a is the semi-major axis of the orbit. Simply plug in the values for G, M1, M2, and a to find the orbital period.
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Neptune, at about 165 Earth years.