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The term precession of the equinoxes refers to the fact that Earth's spin axis does not stay fixed, but instead sweeps out a cone once every 26,000 years. (This explains why our pole star, Polaris, will not remain the pole star forever.) The reason for this instability is that Earth is a giant gyroscope. The spin axis of Earth precesses because of the torques exerted on it by the gravitational forces of the Sun and moon. The angle between the direction of Earth's spin axis and the normal to the ecliptic plane (the plane of Earth's orbit) is 22.5 degrees.

The term precession of the equinoxes refers to the fact that Earth's spin axis does not stay fixed, but instead sweeps out a cone once every 26,000 years. (This explains why our pole star, Polaris, will not remain the pole star forever.) The reason for this instability is that Earth is a giant gyroscope. The spin axis of Earth precesses because of the torques exerted on it by the gravitational forces of the Sun and moon. The angle between the direction of Earth's spin axis and the normal to the ecliptic plane (the plane of Earth's orbit) is 22.5 degrees.

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The term precession of the equinoxes refers to the fact that Earth's spin axis does not stay fixed, but instead sweeps out a cone once every 26,000 years. (This explains why our pole star, Polaris, will not remain the pole star forever.) The reason for this instability is that Earth is a giant gyroscope. The spin axis of Earth precesses because of the torques exerted on it by the gravitational forces of the Sun and moon. The angle between the direction of Earth's spin axis and the normal to the ecliptic plane (the plane of Earth's orbit) is 22.5 degrees. What is the approximate value for this torque t, given that the period of rotation of Earth is 1.00 day and its moment of inertia is 8.03 × 10³7 kg⋅m²? T = 4.5 ×1023 Incorrect N.m
Transcribed Image Text:The term precession of the equinoxes refers to the fact that Earth's spin axis does not stay fixed, but instead sweeps out a cone once every 26,000 years. (This explains why our pole star, Polaris, will not remain the pole star forever.) The reason for this instability is that Earth is a giant gyroscope. The spin axis of Earth precesses because of the torques exerted on it by the gravitational forces of the Sun and moon. The angle between the direction of Earth's spin axis and the normal to the ecliptic plane (the plane of Earth's orbit) is 22.5 degrees. What is the approximate value for this torque t, given that the period of rotation of Earth is 1.00 day and its moment of inertia is 8.03 × 10³7 kg⋅m²? T = 4.5 ×1023 Incorrect N.m
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