DATA Navigating in the Solar System . The Mars Polar Lander spacecraft was launched on January 3. 1999. On December 3. 1999, the day Mars Polar Lander impacted Martian surface at high velocity and probably disintegrated, positions of the earth and Mars were given by these coordinates: With these coordinates, the sun is at the origin and the earth’s orbit is in the xy -plane. The earth passes through the + x -axis once a year on the autumnal equinox, the first day of autumn in the northern hemisphere (on or about September 22). One AU, or astronomical unit , is equal to 1.496 × 10 8 km, the average distance from the earth to the sun. (a) Draw the positions of the sun, the earth, and Mars on December 3. 1999. (b) Find these distances in AU on December 3. 1999: from (i) the sun to the earth, (ii) the sun to Mars; (iii) the earth to Mars, (c) As seen from the earth, what was the angle between the direction to the sun and the direction to Mars on December 3. 1999? (d) Explain whether Mars was visible from your current location at midnight on December 3, 1999. (When it is midnight, the sun is on the opposite side of the earth from you.)
DATA Navigating in the Solar System . The Mars Polar Lander spacecraft was launched on January 3. 1999. On December 3. 1999, the day Mars Polar Lander impacted Martian surface at high velocity and probably disintegrated, positions of the earth and Mars were given by these coordinates: With these coordinates, the sun is at the origin and the earth’s orbit is in the xy -plane. The earth passes through the + x -axis once a year on the autumnal equinox, the first day of autumn in the northern hemisphere (on or about September 22). One AU, or astronomical unit , is equal to 1.496 × 10 8 km, the average distance from the earth to the sun. (a) Draw the positions of the sun, the earth, and Mars on December 3. 1999. (b) Find these distances in AU on December 3. 1999: from (i) the sun to the earth, (ii) the sun to Mars; (iii) the earth to Mars, (c) As seen from the earth, what was the angle between the direction to the sun and the direction to Mars on December 3. 1999? (d) Explain whether Mars was visible from your current location at midnight on December 3, 1999. (When it is midnight, the sun is on the opposite side of the earth from you.)
DATA Navigating in the Solar System. The Mars Polar Lander spacecraft was launched on January 3. 1999. On December 3. 1999, the day Mars Polar Lander impacted Martian surface at high velocity and probably disintegrated, positions of the earth and Mars were given by these coordinates:
With these coordinates, the sun is at the origin and the earth’s orbit is in the xy-plane. The earth passes through the +x-axis once a year on the autumnal equinox, the first day of autumn in the northern hemisphere (on or about September 22). One AU, or astronomical unit, is equal to 1.496 × 108 km, the average distance from the earth to the sun. (a) Draw the positions of the sun, the earth, and Mars on December 3. 1999. (b) Find these distances in AU on December 3. 1999: from (i) the sun to the earth, (ii) the sun to Mars; (iii) the earth to Mars, (c) As seen from the earth, what was the angle between the direction to the sun and the direction to Mars on December 3. 1999? (d) Explain whether Mars was visible from your current location at midnight on December 3, 1999. (When it is midnight, the sun is on the opposite side of the earth from you.)
According to Lunar Laser Ranging experiment the average distance Lm from the Earth to the Moon is approximately 3.97 x 105 km. The Moon
orbits the Earth and completes one revolution relative to the stars in approximately 27.5 days (a sidereal month).
Calculate the orbital velocity of the Moon in m/s.
According to Lunar Laser Ranging experiment the average distance LM from the Earth to the Moon is approximately 3.92 x 105 km. The Moon orbits the
Earth and completes one revolution relative to the stars in approximately 27.5 days (a sidereal month).
Calculate the orbital velocity of the Moon in m/s.
Answer:
Choose...
According to Kepler's third law of planetary motion, the mean distance D, in millions of miles, from a planet in our solar system to the sun is related to the time P, in years, that it takes for the planet to
complete a revolution around the sun, and the relationship is
D =
93P2/3
It takes the planet Pluto 248 years to complete a revolution around the sun. What is the mean distance from Pluto to the sun? What is the mean distance from Earth to the sun? Give your answers to the
nearest million miles.
from Pluto to the sun
X million miles
from Earth to the sun
million miles
Chapter 1 Solutions
University Physics with Modern Physics (14th Edition)
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