Calculate the redshift of a star if H-ß line of hydrogen from the star is observed to be 800 nm.
Q: Many of the bright stars in the night sky are highly luminous normal blue stars (such as Acrux), and…
A:
Q: Problem 3: Two stars, M and N, from the same galaxy (at the same distance from earth) are observed…
A: The both stars emit same amount of energy per unit time. Luminosity is given as L=4πR2σT4, where R…
Q: star with mass m, period Ti = 30 days, and radius ri = 1E4 km collapses into a neutron star (Links…
A: Given that The initial radius of the stat ri = 1.0×104Km and Time…
Q: Consider a star whose density increases toward its center. If we model this star as a series of…
A:
Q: A He-Ne laser with wavelength 632.8 nm is fired from a great distance toward a neutron star with…
A: As per the general theory of relativity, gravity affects light and causes energy change in photons.…
Q: Given a 10 Jy source with an occupying 15'' in the sky, at a distance of 1.1 Mpc, observed at 1.4…
A:
Q: The Stelan Bomann equation can be used to estimate the size of asteroids. "Sigma," the…
A: In case of a Black body radiation, Stefan-Boltzmann's law relates the radiant emittance of the black…
Q: What is the escape velocity Vesc of a 1.4M⊙ neutron star if its radius is 12 km? Express your answer…
A:
Q: 1.0 0.8 0.6 Cosmic background data from COBE 0.4 0.2 0.0l 0.5 10 Wavelength A in mm c) The left hand…
A: from the graph, the maximum intensity of radiation is at λ=1 mm. From Wein's law, we have…
Q: Find the wavelength of peak intensity for a hot 45000 K star that emits thermal radiation.
A: Given that:Temperature of the hot star : (T) =45000 K Now, From Wien’s displacement Law…
Q: The surface temperature of a star is measured to be 6000 Kelvin. According to Wien's Displacement…
A: Surface temperature (T) of the star = 6000 Kelvin
Q: Use t = to compute the life expectancy of a 0.9-solar-mass star. (A solar lifetime is approximately…
A:
Q: Find the speed for a star in which this line appears at wavelength 121.8 nmnm. Express your answer…
A: Given that-- (lemda)star = 121.8 nm (lemda) = 121.6 nm Speed of light (c) = 3 × 108 m/s Question?…
Q: At rest hydrogen has a spectral line at 149nm. If this line is observed at 144nm for the star…
A: Given:hydrogen spectral line at rest, λs = 149 nmobserved spectral line, λ = 144 nmAsked:What is the…
Q: The H-alpha line from a star is observed to be 725 nm. Estimate its redshift.
A: As per De Broglie's hypothesis light can behave both as a wave and particle. Thus light waves can…
Q: If a neutron star has a radius of 9.12 km and a temperature of 3.63 x 106 K, how luminous is it in…
A: 1)Using stefan's lawP = σ A T4Where P is the power σ is the stefan's constant A is the area of…
Q: Neutrinos are experimentally determined to have an extremely small mass. Huge numbers of neutrinos…
A: A neutrino may be a sub-atomic particle, which is emitted during the decay. It can uncharged…
Q: To find the Sun’s luminosity from its brightness using the inverse-square law, you also had to be…
A: The distance to the sun can be calculated using the method of parallax. Parallax is defined as the…
Q: 13) Calculate the luminosity in watts from the absolute magnitude for the given stars: (a) Vega (M =…
A: The energy radiated per unit of time by an astronomical object is called luminosity. The…
Q: A supernova occurs 140,000 light years from Earth, where a neutron star of mass 1.6 solar masses and…
A:
Q: What is the maximum luminosity for star of 5.76×1010 Msun.
A: In hydrostatic equilibrium, the radiation pressure and gravitational force will balance each other.…
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: Consider a spherical blackbody of constant temperature and mass M whose surface lies at radial…
A: As per General relativity gravity is capeable causing time dilation. Closer the clock is to the…
Q: Find the speed for a star in which this line appears at wavelength 122.5 nmnm.
A: Given wavelength = 122.5 nm Hydrogen transition wavelength = 121.6 nm Speed of light is c = 3×108…
Q: An x-ray photon escapes the accretion disk of a black hole of 5 solar masses and a radius of 14.7…
A: As per general relativity due to space-time curvature, the frequency of the photon will reduce as it…
Q: A star is observed to be thrice the size of the Sun with temperature of 1.3Tsun. Estimate its…
A: The energy radiated by a star is defined as its luminosity. Luminosity depends on the temperature…
Q: Find the wavelength of peak intensity for a hot 45000 K star that emits thermal radiation.
A: Given in question that Temperature of the object(T) = 45000 K.
Q: An O8 V star has an apparent magnitude of +2. Use the method of spectroscopic parallax to estimate…
A: The apparent magnitude m of the star is given to be m=+1. From HR absolute magnitude M of a star…
Q: If the expanding layers of a supernova move at a constant velocity of v = 10, 000 %3D km/s and the…
A: Given: velocity of supernova v=104 km/s mass of the supernova M=2.4×1031 kg Ephoton=mc2 Time taken…
Q: V603 Aquilae was a nova outburst that occurred on June 8, 1918, at which time it attained a peak…
A: Given information: The apparent magnitude of the (m) = -0.5 The apparent angular diameter of shell…
Q: If gravitational contraction were responsible for the Sun's energy, how long would it take for the…
A: Gravity is one of the fundamental forces of nature responsible for keeping anything with mass…
Q: What is the orbital period (in s) of a bit of matter in an accretion disk that is located 6 ✕ 105 km…
A: Write the given values with the suitable variables. r=6×105 km=6×108 mM=99Mo=992×1030 kg=198×1030 kg…
Q: n hydrogen, the transition from level 2 to level 1 has a rest wavelength of 121.6 nm. Find the speed…
A:
Q: The figure above shows the light-curve obtained from continuous monitoring of the flux received from…
A: Given Star mass Mstar = 1.47 M⊙ Star radius Rstar = 1.84 R⊙ Mass of sun M⊙…
Q: Calculate the surface temperature of the star Betelgeuse whose λmax is 850 nm
A: Wien's Law of Blackbody Radiation λmaxT = a constant = 3 × 106 where λmax = wavelength of radiation…
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: 2. (a) Find the virial mass of a cluster for which the rms radial velocity dispersion is 5 km/s and…
A: Because of how clusters are prepared, they remain as tiny particles in the course of an experiment…
Q: Calculate the Eddington limit for star of 10³0 Msun.
A: In a star, the radiation pressure is constantly pushing away matter while gravity is pulling it in.…
Q: The red supergiant star Betelgeuse has an absolute magnitude of -5.85. If the Sun has an absolute…
A: Luminosity is nothing but intrinsic property. This is the brightness of star which it possesses and…
Q: The surface temperature of a class O blue-white star is around 40 *10^3 K. At what frequency will it…
A: Given data: Surface temperature of class O blue-white star is, T=40×103 K.
Q: Calculate the surface temperature of the star (in K), if the radius of the star is 9,7x10 m and the…
A: Given values: Radius of the star, R=97×108 mMass lost by the star per second, m=54×1010 kg
Q: What is the wavelength in micrometers of peak emission for a black body at 33.5°C? (c = 3.0 × 108…
A: Given values:Temperature of the black body:T = 33.5°C = 306.65 K Wein's displacement law:We know…
Q: What is the peak wavelength (in nm) of a neutron star's luminosity if its temperature is
A: Given that,Temperature : T = 106 (K)Now,As we know that,Using wein's displacement law : λmax T = b…
Q: Distances to the nearest stars (up to 500 ly away) can be measured by a technique called parallax,…
A: The distance between the Sun and the Star is given as, dS = 4 light year (or) dS = 3.784×1013 km TO…
- Redshift happens when the source is moving away from the observer. This will make the observed wavelength longer than the actual one. Since longer wavelength corresponds to red regions we call it redshift.
- Redshift from wavelength is calculated using the following formula,
Here λobs is the observed wavelength and λemit is the emitted wavelength.
Step by step
Solved in 3 steps