OrbitalMotionSE+(1)

1. using Newton’s Law of Universal Gravitation and some kinematics calculation we can calculate the mass of the planet. For this, use this equation in the image:   Given: - vmax = 1.5 m/s - Pstar = 3.5 days  - Mstar = 1.148 Msun, where Msun = 1.98847×1030 kg. This calculation is not shown.

Astronomy help please

10. Match Kepler Laws with the correct description. Kepler's First Law Kepler's Second Law Kepler's Third Lav A planet sweeps out equal areas in equal time frames as it orbits the Sun. Orbits are ellipses with the Sun at a focus. The orbital period is related to the average distance from the Sun. 20 points

2. The generalized Kepler orbit is given in polar coordinates r($)=c/(1+e cos()), where c is a constant and & is the eccentricity of the orbit. Rewrite this in Cartesian coordinates for -1 and show that the orbit is a parabola, y² = A + B x, where A and B are constants. Define constants A and B via constant c.

please don't reject, this is not about astronomy* How was it possible for the Copernican model of the universe to account for the complicated motion of the planets?  PLEASE DO A CLEAR AND UNDERSTANDABLE ANSWER.

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Astronomy help please

I hope you answer this:) 1. Ancient civilizations observed and kept track of daily movement of heavenly bodies. Which one is NOT the reason for this? a. navigation purposes b. time keeping c. annual cultural cycles d. agricultural cycles   2. What Kepler's Law of Planetary Motion is related to the Newton's Law of Motion based from the statement below: The statement: "Since the planets move on ellipses they are continually accelerating." a. Law of Ellipses and Law of Acceleration b. Law of Ellipses and Law of Inertia c. Law of Equal Areas and Law of Interaction d. Law of Period and Law of Inertia e. Law of Period and Law of Acceleration   3. Edwi Hubble proposed a way to organize galaxies in 1920. How are galaxies classified? a. color of stars b. shape of galaxy c. age of stars d. composition of stars e. diameter of galaxy   4. Find the magnifying power (M) and the length (L) of a simple telescope with 30-inches focal length of the objective and 2 inches focal length of the eyepiece.…

Question 1 (Total: 30 points) a. What is a repeat ground-track orbit? b. Explain why repeat ground-track and Sun-synchronous orbits are typically used for Earth observation missions. c. The constraint for a Sun-synchronous and repeat ground-track orbit is given by T = 286, 400, where I is the orbital period in seconds, m the number of days and k the number of revolutions. Explain why this is, in fact, a constraint on the semi-major axis of the orbit.

number 4 please

41. Suppose the orbit of a planet is an ellipse of eccentricity e = c/a and period T (Figure 2). Use Kepler's Second Law to show that the time required to travel from A' to B' is equal to T B b Sun A' a (c, 0) B' FIGURE 2

This is a practice questions for my class. What would this sketch look like? Help me figure it out

Kepler's laws of planetary motion 6. Halley's Comet has an orbital eccentricity of 0.967 and a perihelion distance of 89,000,000 km. (a) Find the orbital period. (b) Find the comet's speed at perihelion and aphelion. 7. Show that the orbital period of a satellite close to the surface of a spherical object depends on the mean density of the object, but not on its size. Find this period for the Earth (density 5.51 g cm-3).

Ma years, what is 2. Saturn has an orbital period of 29.46 years, and its average distance to the sun is 9.54 A.U. If Venus has an orbital period of 0.62 its average distance to the sun in astronomical units (A.U.)? M stance A.U., Conceptual Physics Reading and Study Workbook Chapter 14

The planet Mercury takes 0.24 sidereal years to go around the sun. What is the distance from the center of Mercury to the center of the sun? (Remember 1 sidereal year = 1 revolution) * Your answer The Planet Jupiter's mean orbital radius is 5.2025 AU's. What is the period of Jupiter in Earth years? Your answer There is belt of asteroids between Mars and Jupiter which circles the "inside" of our solar system. This "Asteroid Belt" has a mean radius from the Sun of 2.6 AU's. How long does it take for one asteroid in the belt to travel around the Sun once? * Your answer

1)If the Moon were twice the distance from Earth than it currently is, the amount of time it would take to go around Earth would be roughly (the current orbital period of the Moon is four weeks) Group of answer choices A.eight weeks. B.11 weeks. C.six weeks. D.88 weeks.   2)A satellite is in orbit around a planet. The orbital radius is 46 km and the gravitational acceleration at that height is 7.09 ms-2 . What is the satellite's orbital speed in m/s? (with step)

The Universal Law of Gravitation a. How does halving the distance between two objects affect the gravitational force between them? b. Suppose the Sun was somehow replaced by a star with five times as much mass. What would happen to the gravitational force between the Earth and the Sun? c. How long would the Earth year last in this last case? (hint: Newton’s version of Kepler’s 3rd Law)

1) Calculate the tidal force (the difference in gravitational force from right to left side or G(R) - G(L) ) from a person sitting next to you (approximately 1 meter away). You will need to make some estimations on mass and size of a normal person. 2) Compare the tidal force on a person from the Moon and a person standing nearby (the answers to the previous two questions). Which is greater and by how much?

please don't reject, this is not about astronomy* How was it possible for the Copernican model of the universe to account for the complicated motion of the planets?

Predict the time for Mars to orbit around the Sun if the orbital distance of Mars is1.52 times of Earth`s orbital distance. Note: Earth`s orbital distance (T1) = 1, and Earth`s orbital period (a1) = 1 year. Express your answer in the unit year.   pls help me thankyou

8) The figure shows a planet traveling in a clockwise direction on an elliptical path around a star located at one focus of the ellipse. When the planet is at point A, describe what is happening to the speed of the planet. (Speeding up, remaining the same, slowing down). Explain what principle you use to make answer this question. travels clockwise STAR

1. Which planetary model allows a scientist to predict the exact positions of the planets in the night sky over many years?               2. Which object orbits Earth in both the Earth – centered (geocentric) and Sun – centered (heliocentric) models of our solar system?               3. What is the actual shape of the Earth’s orbit around the Sun?

Johannes Kepler worked as an assistant to the observatory of Brahe at the age of 27. Brahe collected astronomical observations, which were passed into Kepler, on his death. Among the significant contributions of Brahe: 1. His observations on the planetary motion of Mars were used by later astronomers, including Kepler to construct the present model of the solar system. 2. In 1572, he observed supernova as a star that appeared suddenly, became visible for 18 months before it faded from view. Nowadays, supernova is called an exploding star. 3. In 1577, he observed a comet by measuring its parallax. His claim contradicted the idea of Aristotle that comets are "gases burning in the atmosphere." By measuring the parallax for the comet, he was able to show that the comet was further away than the Moon. 4. His findings that stars do not have parallax, he concluded that either: (a). the earth was motionless at the center of the universe; or (b). the stars were so far away that their parallax…

4 My Drive - Google X M You've been offere X O MyFile - Advising S Physics, Neson 12 x G google translate - x eativebookpublishing.ca/books/Nelson-Physics-12.pdf 285 / 746 293% pdf.746 - 12 חכ Sun midway between the orbits of Mars and Jupiter. Determine, to three significant digits, (a) the period of the asteroid's orbit in Earth (b) the asteroid's speed years 35. Scientists want to place a satellite in a circular orbit around Neptune with an orbital period of 24.0 h. (a) Determine Kepler's third-law constant for Neptune using Neptune's mass. (b) What distance from Neptune's centre must the satellite be to maintain its circular orbit? (c) What is the altitude of this orbit in kilometres? 1:1

20) Planet Dwovy circles its star at a distance of 8.75 × 109 km once every 325 Earth years.  The planet Spitnik   circles the same star at a distance of 76.1 × 109 km. What is the orbital period of Spitnik in Earth years? a) 65,800 years b) 2570 years c) 0.004 years d) 8336 years e) 257 years

1. How does the speed of revolution depend on its distance from the sun? 2. How were tycho brahe's observaions used by kepler to produce his laws of planetary motion?

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Find time period only

Directions: Choose the letter that corresponds to the best answer. 1. He is the scientist or philosopher responsible for the theory that proposed that planets, as well as the sun and the moon, moved in a circular motion around the earth.A. Claudius Ptolemy B. Copernicus C. Galileo D. Kepler 2. The following statements are reasons why the geocentric theory was believed or remained unquestioned for more than one (1) millennium, EXCEPT:A. This belief was aligned with the teachings of the church; thus cannot be questioned.B. Majority of the famous philosophers during that period in history supported the idea.C. There was no evidence to prove otherwise due to lack of astronomical instruments.D. People were busy with politics and economics hence it is the least of their concern. 3. Why were most intellectual ideas controversial?A. They challenge the long-held belief and the established institutions.B. They resulted to revolutions and public outcry against governments.C. Many of these ideas…