A binary system is composed of two identical stars orbiting each other with some period To. a) Now imagine scaling all lengths (separation between the stars and the radius of the stars) by a factor k, but keeping the density of the stars the same. By what factor does the period change? b) Now instead of scaling the lengths, scale the density by k (i.e. p → kx p). By what factor does the period change?
Q: If the Earth had twice the radius but the same density (assume constant density), then the…
A:
Q: A star, which is 2.3 x 1020 m from the center of a galaxy, revolves around that center once every…
A:
Q: Figure m 1 of 1 Part A Calculate the angular momentum of a particle of mass m moving with constant…
A:
Q: A star, which is 1.9 x 1020 m from the center of a galaxy, revolves around that center once every…
A: Distance of the star from center of a galaxy (r) = 1.9 × 1020 mTime taken by the star to revolve…
Q: A laser rangefinder is locked on a comet approaching Earth. The distance g(x), in kilometers, of the…
A: Given: funtion g(x)= 350000*cosec((π/30) *x) range x=[0,35] 1. value of function for x= 0+ , g( 0+)…
Q: value. (104, 106.8) 100- 80- (57,63.8) 60+ (68, 63.8) 40+ 20- 20 40 60 80 100
A: This problem can be solved using calculus or from the properties of the graph itself. Here I am…
Q: A very massive star with an M mass has a geometric shape of a sphere hollow, where the mass is…
A:
Q: For the graph of vx versus t shown, estimate the following: i) What is the slope of the tangent line…
A: The above problem can be solved in two different ways. The first method using the two-point formula…
Q: a) Compare the average kinetic energy K,TRT of air molecules to the difference in gravitational…
A:
Q: 100% E toSave OFF 251 Test 2 Study Problems SP20 ans -Saved to my Mac t Draw Design Layout…
A:
Q: The Small Magellanic Cloud is a dwarf galary orbiting the Milky Way at a distance of 50 kiloparsecs…
A: Given: The observed velocity of the Small Magellanic cloud relative to the Milky way is v = 207 km/s…
Q: The mean anomaly of the Pluto was 12.140 degree on July 1st in 1998. The eccentricity of the Pluto…
A: Given, Mean anomaly, M=12.14 Eccentricity, e=0.249 According to Kepler's equation the eccentric…
Q: Please answer within 90 minutes.
A: Step 1: Step 2: Step 3: Step 4:
Q: It is believed that there is a black hole with a mass of approximately four million times the mass…
A:
Q: Find the mass of the block 0 <x< 4,0 < y< 8,0 < z< 1, whose density 8, is given by 8 = 2 – z for 0)…
A: The density is given by: ρ=2-z The mass of the block is calculated as:…
Q: 1. In this problem you will prove that the shortest distance between two points is a line using the…
A:
Q: Plaskett's binary (also known as HD 47129) in the constellation Monoceros is a star system of two…
A: Given: Orbital speed of the stars = 250 km/sec = 250,000 m/s Period of the star = 14.4 days Suppose…
Q: The planet Saturn has an average radius of 9 Earth radii and a density of 0.7 g/cm3 (yes, less dense…
A: The distance at which a moon can orbit a planet without disintegrating by its tidal forces is called…
Q: Centauri A and Centauri B are binary stars with a separation of 3.45 x 10¹2 m and an orbital period…
A: The distance of separation is d= 3.45 x 1012mThe orbital perion is T = 2.52 x 109s
Q: Part A Tangential velocity is velocityA) parallel to the surface of the Earth.B) perpendicular to…
A: (a) Tangential velocity is the linear velocity attributed to a body moving in a circular path. At…
Q: Around 2.5 centuries ago, several physicists of the time came up with the notion of a dark star.…
A: Escape velocity is the minimum velocity required for an object to escape from the gravitational…
Q: A star, which is 2.2 x 1020 m from the center of a galaxy, revolves around that center once every…
A:
Q: One way that astronomers detect planets outside of our solar system (called exoplanets) is commonly…
A: The radial-velocity method for detecting exoplanets relies on the fact that a star does not remain…
Q: The star Sirus A has a mass of 2.06 MO and a radius of 1.71 RO, where M0 is the mass of the Sun…
A:
Q: A planet has a mass of M1, a radius of R1, and a density of ρ1. A second planet has a mass of M2, a…
A:
Q: In 1999, scientists discovered a new class of black holes with masses 100 to 10,000 times the mass…
A:
Q: what would the derivation be for y= Voy(delta t) - .5g(delta t)2
A: here the case is given for an object in free fall motion along the Y axis. Velocity is defined as…
Q: In the deep space between galaxies, the number density of atoms is as low as 106 atoms/m3, and the…
A: Given data NV=106 atom/m3T=2.7 KKB=1.38×10-23 J/KNA=6.023×1023 mol-1
Q: Q 2 Within a certain distance of a black hole, not even light can escape. This distance is called…
A: According to the question the black hole has same mass as the sun Mb = 2.0 x 1030kg since the…
Q: A probe of mass 100 kg is coasting through a dense gas cloud in deep space, where g = 0. There is…
A: Using Newton’s second law of motion mdvdt=Fdmdvdt=-0.6v∫vivfdvv=∫-0.6mdtlnvfvi=-0.6tm
Q: Answer the question in full details, thank you very much, Answer on the correct significant figures:…
A:
Q: The answer key to this problem is stated as follows: x(t) = (4.0 cm)cos[(2π/8.0 s)t - π/3.0] Did…
A: On the 2nd page of answer there was a mistake. cos-1ϕ=12thus ϕ can have values of 600 or -600i.e.…
Q: A star with mass m = 2.624 x 1030 kg revolves around the center of mass of the Milky Way galaxy in…
A: Given, Radius of orbit is 3.7*1020 meter and velocity is 400,000 m/s
Q: In the relativistic free electron gas, the classical kinetic energy E = p²/2m is replaced by E =…
A: It is known that the kinetic energy for relativistic free electron is calculated as, E=p2c2+m2c4-mc2…
Q: The following quotation is taken from the article "Quantum Black Holes", by Bernard J. Carr and…
A: Given that: The total time for a black hole to evaporate away proportional to the cube of itsinitial…
Q: Captain James T. Kirk of Star Trek fame spent a large portion of his time mining for planets that…
A: The radius of the planet=rThe period of the orbit=TMass of ship=mThe minimum distance of his ship…
Q: Here q, = 10 µC, q2 = -5 µC, and q3 = 5 µC. The distance is a = 1 mm. Calculate the force on 93. You…
A: Given that, the value of charge q1 and q2 and q3 and distance (a) is also given. Then We have to…
Trending now
This is a popular solution!
Step by step
Solved in 2 steps
- You also arrested me on the suspicion of art theft. I profess innocence, claiming that I forged a copy of the egg, and so I can’t be accused of stealing a copy that I made. How do you determine whether the egg is a copy or a real work of art? You know that the real Fabergé Egg is mostly hollow, while the “fake” egg may not be. You can model the egg as a cylindrical object (because modeling a real egg is complex), and roll it down an inclined plane. Measuring its velocity at the bottom of the inclined plane will allow you calculate the moment of inertia of the egg, which you can compare to the moments of inertia for a solid cylinder (a disk) and for a hollow cylinder (a hoop). You perform the experiment using a ramp 0.5 m high at one end. You measure the mass of the egg at 400 g and its maximum radius at 9 mm. After several trials, you determine the average velocity of the egg at the bottom of the ramp is 2.56 m/s. Am I going down for art theft?For a 100 kg satellite orbiting Earth in a circular orbit of radius 6500 km, determine the following: Part A its kinetic energy, K Enter your answer in scientific notation in the following format: The coefficient, followed by the capital letter E, followed by the exponent. For example, if your answer is 5.0\times10^8 \space J5.0×108 J, enter 5.0E8 J Part B its potential energy, U (U = 0 at infinity) Enter your answer in scientific notation in the following format: The coefficient, followed by the capital letter E, followed by the exponent. For example, if your answer is 5.0\times10^8 \space J5.0×108 J, enter 5.0E8 JAround 2.5 centuries ago, several physicists of the time came up with the notion of a dark star. This was a star so dense, with so much gravity, that not even light could escape. The calculations used Newtonian mechanics. In class, we calculated the escape speed from the surface of the earth or the distance from the sun, and the mass of the planet or star. Here, the process is partially reversed. Calculate the dark star radius from the mass of the star and the escape speed. Answer in kilometers. c = 3*108 m/s M = 2.4*1030 kg G = 2/3 * 10-10 N*m2/kg2
- ) Several planets possess nearly circular surrounding rings, perhaps composed of material that failed to form a satellite. In addition, many galaxies contain ringlike structures. Consider a homogeneous ring of mass M and radius R. a) What gravitational attraction does it exert on a particle of mass m located a distance x from the center of the ring along its axis? b) Suppose the particle falls from rest as a result of the attraction of the ring of matter. Find an expression for the speed with which it passes through the center of the ring. (a: see notes from class, b: Use the definition of potential energy.)Nothing can escape the event horizon of a black hole, not even light. You can think of the event horizon as being the distance from a black hole at which the escape speed is the speed of light, 3.00×10^8 m/s, making all escape impossible. What is the radius of the event horizon for a black hole with a mass 3.5 times the mass of the sun?Please do this carefully.
- Suppose we represent an ordinary star as a uniform solid rigid sphere. The star’s initial radius is 644000 km (comparableto the size of our sun). After it collapses, forming a neutron star, its final radius is only 18.3 km! If the original starmakes one complete rotation about its axis once per month (every 30 days), find the neutron star’s period of rotationjust after the original star has collapsed.Tafter = (in s)Around 2.5 centuries ago, several physicists of the time came up with the notion of a dark star. This was a star so dense, with so much gravity, that not even light could escape. The calculations used Newtonian mechanics. In class, we calculated the escape speed from the surface of the earth or the distance from the sun, and the mass of the planet or star. Here, the process is partially reversed. Calculate the dark star radius from the mass of the star and the escape speed. Answer in kilometers. c = 3*108 m/s M = 3.2*1030 kg G = 2/3 * 10-10 N*m2/kg2Part A Assuming that these spectral lines correspond to the 656.46-nm hydrogen line in the rest frame, estimate the speed V of the center of mass of the binary system. Express your answer in kilometers per second to three significant figures .Part B Determine the mass M of each star. Express your answer in kilograms to one significant figure.
- Plaskett's binary system consists of two stars that revolve in a circular orbit about a center of mass midway between them. This statement implies that the masses of the two stars are equal (see figure below). Assume the orbital speed of each star is V = 240 km/s and the orbital period of each is 12.1 days. Find the mass M of each star. (For comparison, the mass of our Sun is 1.99 x 1030 kg.) solar masses XCM M2. Integrate the equations of motion for a spherical pendulum, i.e., a particle of mass m moving on the surface of a sphere of radius / in a gravitational field, with Lagrangian L = ml² -(0² + psin² 0) + mglcos 0. 2 Hint: Merely set up the integrals, do not evaluate them. You should obtain two integrals w.r.t. de: one determining t and another determining p. Express the first integral in terms of E,Ueff, m, and l. Express the second integral in terms of E,U eff, m, l, and M₂.Washington, D.C., is located at about 750 W longitude and 380 N latitude. San Francisco is near 1270 W longitude and 380 N latitude. Estimate how many minutes later the Sun rises in San Francisco than inWashington, D. C. How far apart would you estimate these cities to be? Assume that the earth’s radius is 6400 km. One day has 1440 minutes and of course the earth rotates 360 degrees around its axis in one day