Questions tagged [variable-star]
Questions regarding stars that undergo changes in their spectra, temperature, or luminosity.
27
questions
3
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0answers
35 views
What is the theoretical maximum variability a pulsating red giant can have such that a habitable planet can stay habitable for long periods of time?
I was reading about red giants and came across this statement:
Some research suggests that, during the evolution of a 1 M☉ star along the red-giant branch, it could harbor a habitable zone for ...
0
votes
2answers
34 views
Frequency analysis on Semiperiodic object(s) using Lomb-Scargle
So I already did a frequency analysis of the SRv-type's light curve using Period04. I already have the 'periodicities' of the object/star of choice which is quite hard since the latter/other periods ...
2
votes
0answers
51 views
Why do the pulsations of a Cepheid variable occur?
I understand the theory of the mechanism by which Cepheid variables pulsate, where helium is ionised and deionised, leading to changes in diameter.
However, I am unsure if the brightness changes due ...
3
votes
2answers
69 views
Calibrating raw photometric measurements
So I have a photometry data sourced from Solar Mass Ejection Imager's (SMEI) server as an ‘add-on data’ for my point source of interest (a variable star) with a 104 minute cadence. However, it’s not ...
3
votes
2answers
45 views
Delta Velorum - non-observed variable star
I am a beginner variable star observer from the Southern Hemisphere (but with experience in astronomy) and, when I was looking for VS to observe, I saw that Del Vel has almost no observations. Thus, ...
1
vote
0answers
23 views
How do you correct the Period-Luminosity relationship for metallicity?
Refer to the link: https://www.astro.utoronto.ca/DDO/research/cepheids/cepheids.html
Tha author has used the relationship $M_V=-2.902log(P)-1.203$. It is mentioned that this is not corrected for ...
-1
votes
1answer
66 views
How is V1057 Cygni supposed to go from K type dwarf to F type giant?
FU Orionis variables are protostars that go through massive outbursts that drastically change the star's spectral type and magnitude. With the star V1057 Cygni, this star was known to go from a K type ...
2
votes
0answers
54 views
Is Betelgeuse is continually expelling material on the scale of the 2019/2020 event?
The AUGUST 13, 2020 Phys.org article
Results from Hubble suggest that Betelgeuse's recent dimming was due to material ejected from the star says:
...the star's unexpected and significant dimming ...
1
vote
0answers
40 views
Why are the W UMa variable subtypes labelled “A” and “W”?
The W Ursae Majoris variables (eclipsing contact binary stars) are divided into the A- and W-types. As described in Wilson (1978) "On the A-type W UMa systems":
There are two recognized ...
1
vote
2answers
139 views
Why does the Gaia color-magnitude diagram have this shape?
I was looking at the visualization tools of Gaia, and tried plotting a color-magnitude diagram. On the right hand side of the image, photGMeanMag (mag) (the amount ...
2
votes
2answers
63 views
How variable does a star have to be, to be a variable star?
Variable stars are stars whose apparent magnitude varies. But there are so many phenomena that can cause a star to be variable, that I would expect all stars to be variable. A rotating star has a ...
6
votes
0answers
77 views
Color index B-V of the dimming Betelgeuse
Using AAVSO light curve generator I have plotted V and B magnitudes of Betelgeuse in the past 150 days to see trend of B-V color index. If dust would be the cause of the recent drop in the star ...
2
votes
1answer
71 views
What are these data in light curve generator
I'm generating light curves for some variable stars on the AAVSO website (see https://www.aavso.org/lcg ) . I can choose what type of data must be plotted. Can you explain what they are?
Thank you in ...
22
votes
1answer
2k views
Are stars expected to become dimmer before a supernova?
With the recent news about the "fainting" of Betelgeuse and the speculation that this might be a precursor to a supernova, I'm wondering if there is any theoretical/observational basis for this ...
2
votes
0answers
77 views
When we say a variable star is “fainting” does it mean something more or different than “dimming” or “fading”?
A comment below the question Does the current “fainting” of Betelgeuse show any spectral trends that differ from it's normal variability? suggests that "dimming" would be a better term, but I have a ...
5
votes
0answers
163 views
Does the current “fainting” of Betelgeuse show any spectral trends that differ from it's normal variability?
update: With all the newest news about including what the Dr. Becky video discusses as linked in How do magnetic fields mess with astronomers' observations? I'll bet this question can now be ...
1
vote
0answers
113 views
Why do these photometric observations of Betelgeuse look “quantized” in 0.1 magnitude steps?
The most interesting question related to this Will Kinney tweet would be what's going on with Betelgeuse? but I can't help but wonder why much but not all of the photometric data is clustered in ...
2
votes
1answer
70 views
Astrophysics of Supernovae - Energy over Distance?
I need this for worldbuilding, but it is a physics question. I want to be able calculate the energy over distance from a hypernova of a variable star like Eta Carinae. Understanding what energy levels ...
3
votes
1answer
110 views
Brown dwarf magnetic activity
I have not been able to find an answer to my question through google, and therefore ask it on this medium.
Do brown dwarfs have spots and faculae similar to other heavier stars?
3
votes
0answers
25 views
Large amplitude dipole pulsator
Consider a semiregular variable with amplitude of 1.5 mag. Is it possible to explain brightness variations by purely dipole pulsations?
3
votes
1answer
100 views
What is period doubling in a variable star?
I'm coming across the concept of "period doubling" in RR Lyrae stars. When I look up what period doubling is on the Internet, I find general-level explanations of bifurcations of dynamical systems ...
2
votes
1answer
116 views
Are stars beyond the asteroid belt less constant?
If we graph the variability of a small bright star which is lined up with the asteroid belt, is it less constant than stars that are far away from the asteroid belt? To what degree does variability ...
0
votes
1answer
120 views
Stopping down a telescope to reduce brightness by 5 magnitudes
Suppose we have a variable star with a change in magnitude between maximum and minimum of 5 mag.
How much would you need to stop down a telescope (block some of the area) so that the star at maximum ...
2
votes
1answer
226 views
What leads to increase in opacity in kappa mechanism?
I understand that the kappa mechanism (that leads to star variability) causes an increase of opacity with increasing temperature in partial ionization zones. However, I'm not sure I understand what ...
1
vote
2answers
850 views
Do stars vary their own brightness?
All I could find on the internet was about how stars vary in brightness depending on their distance to Earth, temperature, type of star...
But my question is, can a star can change its brightness.
1
vote
1answer
1k views
How to find a Cepheid's pulsation period using its graph?
Basically, I've been seeing these graphs that say: Cepheid Period-Luminosity Relation and the Period axis is supposed to be "logarithmic";
How does this graph work? Since the luminosity of a star ...
2
votes
1answer
116 views
Variable Types of Stars
I'm trying to decode the Variable Types of stars in the Hipparcos Library. I see there are a number of stars for example :-
EA/AR - Does that mean the star is both a EA(Eclipsing Binary Star) and AR ...
