Suppose you observe a binary system containing a main-sequence star and a brown dwarf. The orbital period of the system is 1 year, and the average separation of the system is 1 AU . You then measure the Doppler shifts of the spectral lines from the main-sequence star and the brown dwarf, finding that the orbital speed of the brown dwarf in the system is 23 times greater than that of the main-sequence star. How massive is the brown dwarf in kg?
Q: A (relatively) nearby K-type star known as Nu? Canis Majoris has an estimated orbital radius of…
A: Given Data: Orbital radius, r=2.3344×108 km=2.3344×1011 m Time period, T=736.9…
Q: Time From this light curve, we can deduce that... the star has a high mass exoplanet orbiting it the…
A: Solution: The star having an exoplanet orbiting around the star gives a periodic symmetric variation…
Q: Consider a star whose density increases toward its center. If we model this star as a series of…
A:
Q: What is the average density of a neutron star that has the same mass as the sun but a radius of only…
A:
Q: After the Sun exhausts its nuclear fuel, its ultimate fate may be to collapse to a white dwarf…
A: (a) The expression for the density of the white dwarf star is, ρ=MV Here, M is the mass of the dwarf…
Q: A spinning neutron star of mass M=1.4 solar masses, constant density, and radius R=10 km has a…
A: Angular momentum per unit mass of the accreting material
Q: What is the average density of a neutron star that has the same mass as the sun but a radius of only…
A: Given, mass of sun = mass of neutron star (m) = 1.989×1030 kg radius = 86.31 km
Q: he spectrum of a star is collected and we find the absorption line of Hydrogen-Alpha (the deepest…
A: We know that the Doppler effect, According to the doppler the formula of the doppler shift of the…
Q: (a) Calculate the average density of the white dwarf (in kg/m). )kg/m³ (b) Calculate the surface…
A:
Q: A cepheid star is located at a distance of 18.7kpc from the Earth and has an apparent visual…
A: Step 1:Step 2:
Q: If you weigh 655 N on the earth, what would be your weight on the surface of a neutron star that has…
A: The gravitational force on Earth is equivalent to the force which the Earth exerts on you.…
Q: What is the acceleration of gravity at the surface if the white dwarf has 1.5 the mass of the sun…
A: Given, Mass of white dwarf, Mw=1.5×Ms=1.5×1.989×1030 kg=2.98×1030 kg, and the radius of the white…
Q: Astronomers discover a binary system with a period of 90 days. Both stars have a mass twice that of…
A: Mass of binary system is given by, M=4π2r3GT2 where, M is…
Q: The Sun's mass is 2.0×1030 kg, its radius is 7.0×105 km, and it has a rotational period of…
A: In this question we have to answer what would be the period of the Sun if it collapses into a white…
Q: From the light and velocity curves of an eclipsing spectroscopic binary star system, it is…
A: Given, The radial velocity of stars A and B, vA=5.4km/svB=22.4km/s a. The ratio of stellar masses,…
Q: A certain binary system consists of two stars that have equal masses and revolve in circular orbits…
A:
Q: Imagine a planet orbiting a star. Observations show a Doppler shift in the star's spectrum of 52 m/s…
A: Given that:
Q: what would its period (in s) be if no mass were ejected and a sphere of uniform density can model HD…
A:
Q: A visual binary is composed of two stars A and B. This visual binary has a rotation period of 59.94…
A:
Q: What is the average density of a neutron star that has the same mass as the sun but a radius of only…
A: Given, mass of sun = mass of neutron star = 1.989 ×1030 kg radius = 84.66 km
Q: Analysis of the spectrum of a solar–mass star shows a periodic back-and-forth shift of its spectral…
A:
Q: 2. 60 million years ago, an asteroid hit the Earth and killed every T-Rex on Earth. That same day, a…
A: To estimate the mass of the star that left the main sequence 45 years ago, let's break down the…
Q: Pluto is considered a binary dwarf planet system with its companion Charon. Pluto has a mass of…
A: The center of mass of a system of particles is the point at which all of the mass of the system can…
Q: An exoplanet revolves around a massive star. The radius of the orbit that the exoplanet has is 4.56…
A: Keplers third law of motion relates the time period of revolution of a moon around a planet or that…
Q: WR 68a is a relatively newly discovered (2015) double-lined spectroscopic binary. It has an orbital…
A: Solution: Calculate the orbital radius of each planet from the given time period and velocity.…
Q: Determining the orbit of the two stars of Kepler-34, also called A and B. These two stars together…
A: For a binary system, the period T is T=4π2a3Gm1+m2 Where a is the semi-major axis, m represents the…
Q: Q1 (ints): A0620–00 is an X-ray binary system, there is a normal star and a compact object. For the…
A: A binary system in astronomy consists of two astronomical objects two stars or a star and an…
Q: Models of the first star-forming clouds indicate that they had a temperature of roughly 150 K and a…
A: It is given that, The temperature is T=150 K. The…
Q: The mass of a star is 1.99·1031 kg and its angular velocity is 1.60E-7 rad/s. Find its new angular…
A: Given data: The mass of the star is m=1.99x1031 kg. The initial angular velocity of the star is…
Q: In 2004, astronomers reported the discovery of a large Jupiter-sized planet orbiting very close to…
A:
Q: The two stars Sirius A and Sirius B orbit their commoncenter of mass. Sirius A has a mass of 4.12 ×…
A: Step 1:first we have to take reference and draw the two mass about to the reference point. Step…
Suppose you observe a binary system containing a main-sequence star and a brown dwarf. The orbital period of the system is 1 year, and the average separation of the system is 1 AU . You then measure the Doppler shifts of the spectral lines from the main-sequence star and the brown dwarf, finding that the orbital speed of the brown dwarf in the system is 23 times greater than that of the main-sequence star.
Trending now
This is a popular solution!
Step by step
Solved in 2 steps
- A black hole is a blackbody if ever there was one, so it should emit blackbody radiation, called Hawking radiation. A black hole of mass M has a total energy of MC2, a surface area of 16πG2M2 / c4 and a temperature of hc3 /16π2kGM. Imagine a black hole in empty space, where it emits radiation but absorbs nothing. As it loses energy, its mass must decrease; one could say it "evaporates." Derive a differential equation for the mass as a function of time, and solve this equation to obtain an expression for the lifetime of a black hole in terms of its initial mass.The absolute magnitude of a star in the Andromeda galaxy (distance 690 kpc) is M = 5. It explodes as a supernova, becoming onebillion (10 9 ) times brighter. What is its apparent magnitude?The Algol binary system consists of a 3.7 Msun star and a 0.8 Msun star with an orbital period of 2.87 days. Using Newton’s version of Kepler’s Third Law, calculate the distance, a, between the two stars. Compare that to the size of Betelgeuse (you’ll need to look that up). Newton’s Version of Kepler’s Law: (M1 + M2) P2 = (4p2 /G) a3 Rearrange the equation to solve for a. Pi, p, is equal to 3.14. IMPORTANT NOTE: Google the value of G (the Universal Gravitational Constant) or look it up in your text. NOTICE THE UNITS. You must convert every distance and time in your equation to the same units, otherwise, you’ll get an incorrect answer. That means you must convert distances to meters, solar masses to kilograms, and time to seconds. When you compare your value to the size of Betelgeuse, it will also help that they are in the same units.
- At the surface of a red giant star, the gravitational force on 1 kg is only 2.2 x 10-3 N. If its mass equals 4 x 1031 kg, what is the star’s radius?After the Sun exhausts its nuclear fuel, its ultimate fate may be to collapse to a white dwarf state. In this state, it would have approximately the same mass as it has now, but its radius would be equal to the radius of the Earth.Calculate the average density of the white dwarf.Calculate the surface free-fall acceleration.Calculate the gravitational potential energy associated with a 6.69-kg object at the surface of the white dwarf.The Algol binary system consists of a 3.7 Msun star and a 0.8 Msun star with an orbital period of 2.87 days. Using Newton’s version of Kepler’s Third Law, calculate the distance, a, between the two stars. Compare that to the size of Betelgeuse (you’ll need to look that up). Newton’s Version of Kepler’s Law: (M1 + M2) P2 = (4p2 /G) a3 Rearrange the equation to solve for a. Pi, p, is equal to 3.14. IMPORTANT NOTE: Google the value of G (the Universal Gravitational Constant) or look it up in your text. NOTICE THE UNITS. You must convert every distance and time in your equation to the same units, otherwise, you’ll get an incorrect answer. That means you must convert distances to meters, solar masses to kilograms, and time to seconds. When you compare your value to the size of Betelgeuse, it will also help that they are in the same units.
- 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)As2You've just discovered a new X-ray binary, which we will call Hyp-X1 ("Hyp" for hypothetical). The system Hyp-X1 contains a bright, B2 main-sequence star orbiting an unseen companion. The separation of the stars is estimated to be 21 milion kilometers, and the orbital period of the visible star is 3 days. (a) Use Newton's version of Kepler's third law to calculate the sum of the masses of the two stars in the system. (Hinr. See Mathematical Insight Measuring Stellar Masses in the textbook) Give your answer in both kilograms and solar masses MS-2.0 x 10^30 kg) Express your answer in kilograms to two significant figures. (b) Express your answer as a multiple of Sun's mass to two significant figures. (c) Determine the mass of the unseen companion.(Hint A main-sequence star with spectral type B2 has a mass of about 10 MSun) Express your answer as a multiple of Sun's mass to two significant figures.
- A Type Ia supernova is observed and achieves an apparent magnitude of m = 19.89 at peak brightness. The absolute magnitudes of Type Ia supernovae at peak brightness are known to be M=−19. Determine the distance to the supernovae in units of Mpc.Let us imagine that the spectrum of a star is collected and we find the absorption line of Hydrogen-Alpha (the deepest absorption line of hydrogen in the visible part of the electromagnetic spectrum) to be observed at 656.5 nm instead of 656.3 nm as measured in a lab here on Earth. What is the velocity of this star in m/s? (Hint: speed of light is 3*10^8 m/s; leave the units off of your answer) Question 4 of 7 A Moving to another question will save this response. 1 6:59 & backsAfter the Sun exhausts its nuclear fuel, its ultimate fate may be to collapse to a white dwarf state. In this state, it would have approximately the same mass as it has now, but its radius would be equal to the radius of the Earth. (a) Calculate the average density of the white dwarf. (kg/m3)(b) Calculate the surface free-fall acceleration.( m/s2)(c) Calculate the gravitational potential energy associated with a 1.36-kg object at the surface of the white dwarf.( J)