The most mass of our Milky Way is contained in an inner region close to the core with radius Re. Because the mass outside this inner region is almost constant, the density distribution can be written as following (assume a flat Milky Way with height so): m rs R. dr) =0. r> Ro (a) Derive an expression for the mass M(r) enclosed within the radius r. (b) Derive the expected rotational velocity of the Milky Way (r) at a radius r. (c) Astronomical observations indicate that the rotational velocity follows a different behaviour: 5/2 Draw the expected and observed rotational velocity into the plot below:
Q: What are potential solutions to the missing satellites problem (i.e. solutions that solve the…
A: Introduction: The dwarf galaxy problem, also known as the missing satellites problem, arises from a…
Q: Assume that we have measured the distance to a close by galaxy, with apparent magnitude m1 = 6, to…
A: I HOPE THIS HELPS YOU 🙏.PLEASE GIVE STUDENT RATING----> IF YOU FOUND IT HELPFUL.
Q: Dark matter Consider the rotation curves of a galaxy with density profile p(r). Assuming that…
A: The objective of the question is to determine the relationship between the density and radius of a…
Q: The most mass of our Milky Way is contained in an inner region close to the core with radius Ro.…
A: Hello. Since your question has multiple sub-parts, we will solve the first three sub-parts for you.…
Q: Andromeda galaxy is the closest large galaxy and is visible to the naked eye. Estimate its…
A:
Q: The rest-frame (natural) Wavelength of the H-a line of hydrogen is 656.3 nm. In the spectrum of…
A:
Q: It can be shown that if an object orbiting a star of mass M in a circular orbit of radius R has…
A:
Q: What is the average density of a neutron star that has the same mass as the sun if the radius of the…
A: Given Data: Radius of neutron star, R=41.591 km=41.591×103 m Mass of neutron star =Mass of sun,…
Q: The most mass of our Milky Way is contained in an inner region close to the core with radius Ro.…
A: Hello. Since your question has multiple sub-parts, we will solve the first three sub-parts for you.…
Q: Consider a star whose density increases toward its center. If we model this star as a series of…
A:
Q: Two galaxies are moving away from each other at 8000 km/sec and are 4x103 light-years apart. It was…
A: The speed or velocity of an object is defined as the ratio between the distance traveled by an…
Q: Distances to local galaxies are determined by measuring the brightness of stars, called Cepheid…
A: Absolute brightness is a constant and is 10 parsecs from Earth whereas measured brightness depends…
Q: e gravitational energy of a pair of colliding galaxies , each of mass 10 Mo separated by a distance…
A:
Q: The most mass of our Milky Way is contained in an inner region close to the core with radius Ro.…
A:
Q: The most mass of our Milky Way is contained in an inner region close to the core with radius Ro.…
A: Given, The radius of the inner region close to the core = R0 As we know that, ρ(r)={ρ0,r≤R0…
Q: The nuclei of some galaxics are thought to contain supermassive black holes with M = 3 x 10°M9. How…
A: The Schwarzschild radius of a supermassive black hole can be estimated using an empirical…
Q: You observe a star orbiting in the outer parts of a galaxy. The distance to this galaxy is known,…
A: Given, The distance of the star from the center of the galaxy: r=19 kpc=19×3.086×1019 m Speed of the…
Q: a) Define the term “standard candle” as used in cosmology b). The flux is defined as f(Dlum) = L…
A:
Q: The most mass of our Milky Way is contained in an inner region close to the core with radius Ro.…
A:
Q: Let m be the magnitude of a galaxy and μ be the magnitude per solid angle of the same galaxy. Show…
A: To prove the given relationship for the magnitude 𝑚 of a galaxy in terms of the magnitude per solid…
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: The most mass of our Milky Way is contained in an inner region close to the core with radius Ro.…
A:
Q: An astronomical image shows two objects that have the same apparent magnitude, i.e., the same…
A: Let the luminosity of the star is Ls= LoLuminosity of Milky Way galaxy, Lm=1011LoLuminosity of…
Q: a) If you were to measure the distances and recessional velocities to nearby galaxies, you would…
A: (a) Introduction: Peculiar motion refers to the motion of an object related to a Galactic rest…
Q: The most mass of our Milky Way is contained in an inner region close to the core with radius Ro.…
A: As per guidelines, the first three sub-parts have been answered.
Q: Observations indicate that each galaxy contains a supermassive black hole at its center. These black…
A:
Q: In a white dwarf, each electron can be considered to be located in a region of size 1.5x10-12 m.…
A: White Dwarf: A small very dense star. A white dwarf is formed when low mass star has exhausted all…
Q: The most mass of our Milky Way is contained in an inner region close to the core with radius Ro.…
A:
Q: (a) Estimate the height (z) above or below the Galactic plane for the globular cluster M13 (1,b =…
A: The galactic plane is the plane on which the majority of a disk-shaped galaxy's mass lies. Distance…
Q: 5.4 In a negatively curved universe containing only matter (2, < 1, K = -1), show that the present…
A: Given, the universe contains only matter and Ωo<1 So scale factor will be a=12ΩoΩo-1coshθ-1…
Q: Distances to very remote galaxies are estimated based on their apparent type, which indicate the…
A: The relation of brightens of the star is inversely proportional to the square root of the distance…
Q: The most mass of our Milky Way is contained in an inner region close to the core with radius Ro-…
A: Hello. Since your question has multiple sub-parts, we will solve the first three sub-parts for you.…
Q: In the deep space between galaxies, the number density of atoms is as low as 106 atoms/m3, and the…
A:
Q: 3. Consider a galaxy at a distance of 1.7 Mpc from Earth, in which the rotational velocity of the HI…
A: Note: Since we only answer up to 3 sub-parts, we’ll answer the first 3. Please resubmit the question…
Q: Our galaxy is approximately 100,000 light years in diameter and 2,000 light years thick through the…
A:
Q: Please answer within 90 minutes.
A: a. Total number of stars in the population b. Surface density wave This is not an integer, so we…
Q: A student in PHYS 115 at NYIT wants to estimate the age of the galaxy. She knows that the most…
A:
Q: To get an idea of how empty deep space is on the average, perform the following calculations: (a)…
A: “Since you have posted a question with multiple sub-parts, we will solve first three subpartsfor…
Q: n(r) = nge where r represents the distance from the centre of the Galaxy, Ro is the distance of the…
A: (a)As we have to find the maximum distance by the help of the relation of absolute and apparent…
Q: On average, how far away are galaxies that are moving away from us at 2.0% of the speed of light?
A:
Q: -0.5 = Compute the Oort constants A and B for Keplerian rotation: 0(R) Oo (R/Ro) in terms of eo and…
A: Solution: The Oort constants are given by the following: A=-dΘdRR0-Θ0R0…
Q: A galaxy is found to be receding at a velocity of 3.0 x 104 km-s-1. Calculate the distance to the…
A: Edwin Hubble discovered through observation that the Universe is expanding. Galaxies are moving away…
Q: The most mass of our Milky Way is contained in an inner region close to the core with radius Ro.…
A: As per guidelines, the first three sub-parts have been answered.
Step by step
Solved in 2 steps with 2 images
- The qs was solved here.urgent plsDerive 5 equations in UARM.The great astronomer Edwin Hubble discovered that alldistant galaxies are receding from our Milky Way Galaxy withvelocities proportional to their distances. It appears to anobserver on the Earth that we are at the center of anexpanding universe.. illustrates this for fivegalaxies lying along a straight line, with the Milky Way Galaxyat the center. Using the data from the figure, calculate thevelocities: (a) relative to galaxy 2 and (b) relative to galaxy 5.The results mean that observers on all galaxies will seethemselves at the center of the expanding universe, and theywould likely be aware of relative velocities, concluding that itis not possible to locate the center of expansion with thegiven information.
- a)Define the term “standard candle” as used in cosmology. b)The flux is defined asf(Dlum) = L/4πD^2lumwhere L is the absolute luminosity and Dlum is the distance to the radiation source (youmay assume z ≪ 1).Assume that we have measured the flux to be f = 7.234 10^−23 Wm^−2 and the absoluteluminosity is given by L = 3.828 x10^26W. Calculate the luminosity distance D lum to the objectin Mpc.Question is in form of picture !You observe a star orbiting in the outer parts of a galaxy. The distance to this galaxy is known, and you are able to take a spectra of this star and determine its velocity. The star is 22 kpc from the galaxy center and moving in a circular orbit with speed 304 km/s. Compute the total mass of the galaxy internal to the star's orbit. You will get a large number; express it in scientific notation and in units of solar masses [e.g., 4.2e10]. [Hint: there is a Box in Chapter 22 of your textbook that will be of help. See also the course formula sheet.]
- The most mass of our Milky Way is contained in an inner region close to the core with radius Ro. Because the mass outside this inner region is almost constant, the density distribution can be written as following (assume a flat Milky Way with height zo): { r Ro Po, p(r) = 0, (a) Derive an expression for the mass M(r) enclosed within the radius r. (b) Derive the expected rotational velocity of the Milky Way v(r) at a radius r. (c) Astronomical observations indicate that the rotational velocity follows a different behaviour: Vobs (r) = VGT Po z0 Ro 5/2 1+e-4r/Ro 4 Draw the expected and observed rotational velocity into the plot below:The CaII H and K lines have rest wavelengths of 396.85 nm and 393.36 nm, respectively. In the spectrum of a galaxy in the cluster Abell 2065, the observed wavelengths of the two lines are 425.50 nm and 421.76 nm. a) What is the redshift z of the galaxy? b) What is the distance to the galaxy? c) What is the distance modulus of the galaxy?The most mass of our Milky Way is contained in an inner region close to the core with radius Ro- Because the mass outside this inner region is almost constant, the density distribution can be written as following (assume a flat Milky Way with height zo): Po, r Ro (a) Derive an expression for the mass M(r) enclosed within the radius r. (b) Derive the expected rotational velocity of the Milky Way v(r) at a radius r. (c) Astronomical observations indicate that the rotational velocity follows a different behaviour: Veda (r) = /G#po:0Ro (- 5/2 1+e-dr/Ro Draw the expected and observed rotational velocity into the plot below: 20 1.5 1.0 10 Radius from Center r [R] (d) Scientists believe the reasons for the difference to be dark matter: Determine the rotational velocity due to dark matter vpM (r) from Ro and draw it into the plot above. (e) Derive the dark matter mass MpM(r) enclosed in r and explain its distributed. (f) Explain briefly three theories that provide explanations for dark matter.…
- The surface mass density of the disk of a galaxy is given in the provided image. Σ0 is the central surface density and Rd is the scale-length, and they are both constant. Find the total mass (M) of the disk in terms of Σ0 and Rd.c. The critical density for the Universe is given by 3H% Pcrit 8TG Calculate the ratio between the values derived for the critical density of the Universe assuming Ho = H5 Planck and Ho = H° = HSHOESNGC 3379 is an El galaxy at a distance of 14.8 Mpc that has an apparent B band magnitude of 10.65 and a central velocity dispersion of 220 kms¬1. M87 is also an El galaxy, but lies in the Virgo cluster. M87 has a central velocity dispersion of 315 km s and an apparent B-band magnitude of 10.1. Assuming that both of these galaxies exactly follow the scaling relation that connects these properties, what is the distance to M87?