Questions tagged [luminosity]
Questions regarding the amount of energy produced by an object per unit of time.
101
questions
-1
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1answer
40 views
How to find luminosity from a light curve? [closed]
I am currently trying to find the luminosity from the light curve. I have the data about the distance, counts/sec and the energy range in which it is measured for an object. What equation can be used ...
5
votes
3answers
610 views
Could a black hole's accretion disk be bright through natural means?
This question is based on this description of the Cormoran Supermassive Black Hole in the Orion Arm's website:
Surrounding this event horizon is an (apparently artificial) accretion
disk about 4AU in ...
5
votes
1answer
98 views
What does a + (plus) mean in stellar classification?
I've noticed some stellar classifications might look like this:
A0IV+G: (HD 70003)
F3IV+F0IV (HD 82434)
...
12
votes
1answer
972 views
Spectral class and luminosity of hydrogen bomb explosions?
Since hydrogen bombs detonating are like tiny little stars, I wonder what luminosity and spectral classification they would get if one were to categorize them like this. E.g. Starfish Prime and the ...
2
votes
0answers
17 views
How to calculate rest-frame luminosity in a specific wavelength band?
For instance, I have a set of templates whose y is in Jy and x is in Angstroms. I have both of their rest-frame and obs-frame wavelength (i.e. redshift). I want to know their luminosity in one ...
4
votes
1answer
96 views
Is it dangerous to look at an L-type brown dwarf from too close?
Are some L-type brown dwarves bright enough so that it would be dangerous to the eyes if one looked at them from habitable distance or closer? If not, are the weakest M-type stars undangerous to look ...
3
votes
1answer
54 views
How is the difference of bolometric magnitudes not dependent on the stars' radii?
The difference of 2 bolometric magnitudes is given by:
$$M_{bol, ★} - M_{bol, ☉} = -2.5 \cdot \log \left( \frac{L_★}{L_☉} \right)$$
But Pogson's equation is:
$$M_{bol, ★} - M_{bol, ☉} = -2.5 \cdot \...
1
vote
1answer
50 views
HR diagram x-axis (color) and redshift?
I've read several articles and watched some videos on the HR diagram, but no-one seems to mention the effect of redshift on the color of a star. Is there some calibration step that needs to be applied ...
0
votes
1answer
47 views
Is something wrong with my luminosity calculation?
A few million years after a white dwarf forms, its surface temperature reaches $100000\text{K}$, while its radius is $0.01R_\odot$. Would this mean that its luminosity is $\Big(\dfrac{100000}{5778}\...
0
votes
1answer
43 views
How to calculate galaxy bolometric luminosity?
I am a bit confused by bolometric corrections. If I have an x-ray luminosity in the 2-10 keV band, how does one convert that to $L_{bol}$?
From Netzer's book The Physics and Evolution of Active ...
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0answers
151 views
Schechter Luminosity Function fitting plot of galaxies
I would like to plot the Schechter Luminosity function of galaxies. Here is my data(I have the Luminosity L[Ha] in erg/s).
I would like to plot like this figure from this paper.
In this paper, they ...
0
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0answers
26 views
How to calculate the luminosity of a quasar?
Is there a relation between the distance ($d$) and the apparent bolometric magnitude ($m_{bol}$) of a quasar and its luminosity ($L$) in watt? If so, what is that relation?
Thanks in advance!
1
vote
1answer
57 views
Estimating Sun luminosity from first principles
In a lecture, it was claimed that luminosity can be estimated by dividing how much energy there is in the Sun with the typical time it takes for a photon to get out from the centre of the Sun to its ...
1
vote
0answers
20 views
Equilibrium Temperature for Extremely Cold Planets: Incorporating the CMB and Intrinsic Radiation
I want to check if I'm doing this right. I'm computing the equilibrium temperature for planets where the CMB and/or the planet's intrinsic radiation (as in weakly radiating jovians) matters.
I start ...
0
votes
1answer
35 views
Does photon capture in a black hole (or any other "very compact" object) reduce the luminosity/photon flux from its self isotropic emission?
I don't know if this is even a feasible question or if I have a point in asking so.
Let's say we can model the radiation coming from a very compact object, such as a BH with an accretion disc or any ...
1
vote
1answer
70 views
How to obtain a luminosity from an SED
I have a spectral energy distribution (flux densities measured at several frequencies), and have fitted a 'greybody' model to these points.
I am confused about how I use this information to determine ...
1
vote
1answer
166 views
What units are used for the Stefan-Boltzmann law?
I have a star with given temperature in Kelvin and radius in solar radii. I tried to calculate the luminosity of the star using Stefan Boltzmann's law, and got an absurd number (over 1 million). What ...
9
votes
1answer
674 views
Increase in Luminosity of the star
The Luminosity of a star is proportional to the 4 th power of its temperature and square of its radius. Also the mass-luminosity relationship says that the luminosity of star is proportional to ...
3
votes
1answer
68 views
Luminosity of Neowise
So, I have been trying to figure out the bolometric luminosity of the comet C/2020 F3 (Neowise) on the 22nd of June, 2020. At that time, Neowise was $1.4$ AU away from Earth and had an apparent ...
0
votes
0answers
35 views
Samples from the double Schechter luminosity funcion
I want to produce samples from a double Schechter luminosity function.
Ideally, I am looking for a python implementation of this problem but am open to other tools if necessary.
Do you know of any ...
8
votes
3answers
155 views
What is meant by the notation $A^{\times{B}}_{\div{C}}$; where A,B,C are real numbers?
I have come across a few papers using the notation $A^{\times{B}}_{\div{C}}$; where A,B,C are real number. For example, $3000^{\times{3}}_{\div{4}}$.
An example can be Eqn (4) in Stern & Laor (...
2
votes
1answer
91 views
Converting Light curve to Luminosity
So I'm currently working around a specific variable star, α Ori and I want to determine it's luminosity...I do only have the light curve (driven from V-optical photometric band - Johnson V from AAVSO)....
2
votes
1answer
74 views
Strip Brightness in a Spherical System
My question concerns the following problem, published in Galactic Dynamics by Binney and Tremaine and based on a work by Schwarzschild.
Specifically, I am having difficulties in deriving the given ...
2
votes
0answers
67 views
How do I calculate the surface temperature of a star from luminosity? [duplicate]
How do I calculate the surface temperature of a star from luminosity? I've been trying to delve into speculative solar systems for a bit, and I've heard the surface temperature of a star can be ...
1
vote
1answer
67 views
How does the Eddington limit make the gravitational field of stars asymmetric?
This answer to Is the gravitational field of the sun uniform? says:
Very large stars are asymmetric due to being close to the Eddington limit. The Sun is too small of a star to have the kind of ...
11
votes
1answer
230 views
Is there a relation between mass, radius, and luminosity in deuterium-burning brown dwarfs?
I'm a worldbuilder and my setting has a lot of brown dwarfs.
While I'm trying to keep my setting as science-compliant as possible, I can't seem to find any resources for brown dwarfs like there are ...
1
vote
0answers
19 views
Total luminosity of total population of galaxies!
I'm trying to get the total luminosity of a total population of galaxies.
I have the Schechter Function like
$$\Phi(L) = \frac{\Phi^{*}}{L^{*}} \left(\frac{L}{L^{*}}\right)^{\alpha} \exp \left(\frac{...
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vote
0answers
130 views
Units confusion while calculating flux of a star using distance and luminosity, Python
I am trying to calculate the flux of various stars in Python. I am using the information from a database containing all stars in Hipparcos, Yale Bright Star, and Gliese catalogs (almost 120,000 stars)....
3
votes
1answer
941 views
Does the luminosity of a star on its main sequence increase or remain approximately constant?
From my understanding, the luminosity of a main sequence star should increase because, in its core, hydrogen is being burnt into helium which means that the number density of hydrogen decreases and ...
7
votes
4answers
1k views
Visible Stars in Andromeda Galaxy
So when I look at images taken of Andromeda, I see a lot of individual stars.
Image by André van der Hoeven
It seems to me that the actual individual stars that far away would be too small to ...
7
votes
1answer
603 views
What is the most appropriate way to estimate the helium composition of a star?
Say we have to estimate the helium content in Proxima Centauri.
We begin by calculating the content of helium in the Sun (source): $24.85$% of $2.10^{30}$ kg.
Mostly all the energy is generated due ...
2
votes
1answer
304 views
How to convert luminosity at rest frame wavelength of 1450 A to absolute magnitude at 1450 A?
How do I convert the luminosity (erg sec$^{-1}$ Hz$^{-1}$) of a quasar at a rest frame wavelength of 1450 Angstroms to absolute magnitude at the same wavelength?
I know that the bolometric ...
2
votes
0answers
240 views
What is the spectral energy distribution (SED)?
I see the SED being referred to as several different things and now I am confused about what it actually is and what are its units. In particular, I find the SED Wikipedia page not understandable.
...
4
votes
1answer
206 views
Convolve a SED with a filter. Is convoluting the mathematical operation?
I know that in order to get the Flux of a star (or something else) in a particular filter from its SED (luminosity per unit wavelength), I need to convolve the spectrum (SED) with the filter response. ...
1
vote
1answer
135 views
Can a star emit a larger fraction of its total light in the visual range than the Sun does
If one sets both the bolometric and visual luminosity of the Sun to 1 (and use a linear scale), can a star then have a higher visual than bolometric luminosity?
It makes sense that this will not be ...
0
votes
0answers
22 views
Relationship between IMF and time spent during an evolutionary phase
I was reading a little about stellar evolution and was wondering whether there was any relationship between the lifetime of an evolutionary phase and the IMF, I searched on google but all I found were ...
2
votes
1answer
626 views
Formula to calculate B-V index? [duplicate]
Is there a formlua or equation to calculate a star's B-V index based on it's observed frequencies in the B and V spectrums ? I have unfortunately not been able to find anything...
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votes
1answer
130 views
Finding the solar radius from temperature and luminosity
This question has eluded me for days; I can't seem to solve it.
A certain star has a temperature twice that of the Sun and a luminosity 55 times greater than the solar value. What is its radius, in ...
4
votes
1answer
483 views
Estimating a star's radius, temperature, and luminosity based on its mass
(See updated figure and description below.)
I've been trying to generate ballpark estimates for the radius, temperature and luminosity of stars in the main sequence based solely on their masses (...
1
vote
1answer
77 views
How Wide Would the Habitable Zone Be in a Singular Red Giant System?
Astrobiologists looking for signs of life outside Earth usually take excitement over planets orbiting red giant stars because a larger, brighter star usually means a farther-away but still wider ...
0
votes
1answer
477 views
Why is the Sun's Luminosity not equal to the Zero Point Luminosity?
I was doing some research and found that the zero-point luminosity was $L_\odot = 3.75\times 10^{28} $, while the sun's reported luminosity was $L_{Sun} = 3.828\times 10^{26}$, according to Wikipedia. ...
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vote
0answers
36 views
How to convert magnitude to spectral luminosity? [duplicate]
In the Gaia catalogue I have the magnitude of several stars in the G band. I also have the distances to these stars (parallax is known). Additionally, I oftentimes have the effective temperature in ...
0
votes
1answer
305 views
Converting the log (Stellar Luminosity/Solar Luminosity) and the log of the plus and minus variation
There are some stars in the NASA Exoplanet Archive that I am interested in but I am confused by the physical meaning of the terms.
For example, there's a star BD+15 2940 with a log10 of Solar ...
1
vote
0answers
197 views
Q: Calculating the luminosity of a galaxy
I am currently working on a project on which I am calculating the luminosity of galaxies by using the SDSS data. They use a system of asinh magnitudes, and according to their website they use a system ...
2
votes
0answers
187 views
Stars that don't fit $L=4\pi R^{2}\sigma T^{4}$?
When calculating luminosity/radius/temperature for several stars, I've noticed that while the majority of stars conform to the luminosity relationship $L=4\pi R^{2}\sigma T^{4}$, there are a few that ...
2
votes
2answers
122 views
How to calculate the distance to galaxies with standard candles?
I was wondering how the distance in Mpc could be calculated between Earth and a galaxy using the luminosity provided? Do not be shy to use all math necessary :)
Clarification:
Luminosity is inversely ...
10
votes
1answer
133 views
How actively is Deep Learning being used in exoplanet identification?
Papers, like this one from Google, show that Deep Learning and Machine Learning are effective in detecting exoplanets from luminosity data provided by telescopes like TESS or Kepler.
These models ...
1
vote
1answer
132 views
Eddington luminosity in various plasmas
So I know that the Eddington luminosity is given by:
$L_{Eddington} = 4\pi GMc/\kappa$.
I want to calculate this luminosity for a plasma of purely ionized helium, as well as for an electron-...
2
votes
2answers
439 views
Radiative Flux, Irradiance and Luminosity confusion
First of all I know there is a similar question here, but I feel is wasn't answered at all.
My question is that I have seen many texts which says that Radiative Flux is equal to the Irradiance of a ...
3
votes
1answer
951 views
How to correct observed flux densities for redshift
Say I have a spectrum of a galaxy at a redshift $z$, in flux density units of erg/s/cm^2/Angstrom. I'd like to recover the spectrum (in the same flux density units) at z=0, i.e. at its rest ...
