(1) Halley's Comet and Kepler's Laws: Halley's Comet orbits the Sun every 76.0 years. Its elliptical...
Suppose Halley's comet orbits the Sun every 67 years and has an eccentricity of 0.95. What is the perihelion distance of Halley’s comet in AU?
A comet has a period of 72.3 years and moves in an elliptical orbit in which its perihelion (closest approach to the Sun) is 0.650 AU. Find the semimajor axis of the comet and an estimate of the comet's maximum distance from the Sun, both in astronomical units. (a.) the semimajor axis of the comet (in AU). (b.) an estimate of the comet's maximum distance (in AU) from the Sun.
PLEASE HELP TO ANSWER THIS LAB ACTIVITY Activity 3: Kepler's Second Law: Objects in elliptical orbits sweep oul equal areas in'equal times. This implies that the orbital speed of a planet around the sun is not uniform - it moves farthest away (known as APHELION). In this section we will calculate the difference in this fastest at the point closest to the sun (known as the PERIHELION) and slowest at the point speed using Pluto as an example. Pluto's orbit...
1. Halley’s Comet moves in an elongated elliptical orbit around the Sun. Its distances from the sun at perihelion and aphelion are 8.75 × 107 km and 5.26 × 109 km, respectively. Find the orbital semi-major axis, eccentricity, and period for Halley’s Comet. 2。 A toboggan loaded with students (total weight 300 kg) slides down a snow-covered slope. The hill slopes at a constant angle 40.0 ◦ , and the toboggan is so well waxed that there is virtually no...
A)Some comets are in highly elongated orbits that come very close to the sun at perihelion. The distance from one such comet to the center of the sun is 6.00×10^9m at perihelion and 3.00×10^12m at aphelion. For this comet's orbit, find the semi-major axis. B) In 2017 astronomers discovered a planet orbiting the star HATS-43. The orbit of the planet around HATS-43 has semi-major axis 7.41×109m, eccentricity 0.173, and period 4.39 days. Find the distance between HATS-43 and the planet...
1 points SPreCalc7112.065.MI. My Notes Ask Your Teacher The planets move around the sun in elliptical orbits with the sun at one focus. The point in the orbit at which the planet is closest to the sun is called perihelion, and the point at which it is farthest is called aphelion. These points are the vertices of the orbit. A planet's distance from the sun is 207,000,000 km at perihelion and 249,000,000 km at aphelion. Find an equation for the...
6.) According to Kepler's Laws, planets have elliptical orbits, with the sun at one of the foci. The farthest Pluto gets from the sun is 7.4 billion kilometers. The closest it gets to the sun is 4.4 billion kilometers. Find the equation of Pluto's orbit assuming a center at (0,0). 7.) An arch in the shape of the upper half of an ellipse is used to support a bridge that is to span a river 20 meters wide. The center...
QUESTION 1: The International Space Station has a mass of 4.19 ✕ 105 kg and orbits at a radius of 6.79 ✕ 106 m from the center of Earth. Find the gravitational force exerted by Earth on the space station, the space station's gravitational potential energy, and the weight of a 92.3 kgastronaut living inside the station. HINT (a) the gravitational force (in N) exerted by Earth on the space station (Enter the magnitude.) N (b) the space station's gravitational...
keplers laws starry night lab questions Kepler EAND DATE Name: Class/Section: and let Xohie. hen it has gone TOwing Eart iginal croing e up X with Sous step. Write Noht Student Exercise-Answer Sheet Keplers Laws hatis the orbital period of asteroid X as calculated from Kepler's law? ete an orbit? Does mitation in at aphelion to a planet's question s agee 2 Describe how the period of the orbit depends on the orbital eccentricity, e. Lebad created an orbit with...
could you please solve a and b? Chapier 2i. Note: you needn't derive Kepler's laws-but do mention when you are using them, an describe the physical concepts involved and the meanings behind the variables. u) Consider two stars Mi and M; bound together by their mutual gravitational force (and isolated from other forces) moving in elliptical orbits (of eccentricity e and semi-major axes ai and az) at distances 11 in n and r from their center of mass located at...