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Unanswered Questions

136 questions with no upvoted or accepted answers
-6 votes
0 answers
70 views

Answer this or don't downvote

Otherwise you'll be showing your complete ignorance in the matter and contempt for the truth. If the scale factor as a function of time represents or is equal to the average distance between the ...
1 vote
0 answers
16 views

cross-matched SDSS-WISE catalog

Please where can I find cross-matched SDSS and WISE dataset for a machine learning project? (Galaxy-star-qso classification task)
2 votes
0 answers
84 views

Would we know if the universe was rotating?

I was wondering what we would observe if the universe had a small rotation. My conclusion was that galaxies on the equatorial plane of the universe would be slightly more redshifted than galaxies than ...
0 votes
0 answers
22 views

how to set a image normalization similar to the default scale for SAOImageDS9 zscale

I want to draw this picture using mmatplotlib, and I want to set the normalization to be Exactly Same as zscale (as in the below image) for example, I can use simple_norm or general ImageNormalize but ...
3 votes
0 answers
41 views

Why MIT's Benjamin Rackham says "nearby ultracool dwarf SPECULOOS-3" would look "purplish-red, spotted, and flaring" from an airless orbiting planet?

May 15, 2024 MIT News article Newly discovered Earth-sized planet may lack an atmosphere includes the following: “We can say from our spectra and other observations that the star has a temperature of ...
1 vote
0 answers
43 views

Tiling the sky with astropy-healpix

I have a bunch of files containing sources with galactic l and b values. What I want is to redistribute the sources such that each new file contain sources that fall within 15 degrees of a central l,b ...
0 votes
0 answers
35 views

Project Analog Hypothetical Planet

For my story Project Analog, I was wondering if a hypothetical planet (Let's call it Suria). It has the same size and conditions as Earth with the same axis, tilt, and rotation, as well as one moon. ...
2 votes
0 answers
102 views

What would the Big Crunch theoretically look/feel like?

In the Big Crunch theory, the expansion of the universe reverses, resulting in all matter contracting into a single point. Imagine you are alive at the time of this event. What would the sky look like?...
2 votes
0 answers
34 views

Local anisotropies in the expansion of the universe and tidal forces...?

In the context of the large-scale structure of the universe, there can be local anisotropies (https://www.aanda.org/articles/aa/full_html/2021/05/aa40296-21/aa40296-21.html). I understand from this ...
2 votes
0 answers
78 views

Gaia coordinates in J2000 as done by the CDS

So I'm interested in knowing how the CDS calculates the J2000 equatorial coordinates from the Gaia DR3 equatorial coordinates (that are given in epoch 2016.0). For example, for the star HD 308819 = ...
0 votes
0 answers
25 views

Deriving Faber-Jackson Relation from Milgrom's Law

I am reading Famaey & McGaugh 2011, a review paper on Modified Newtonian Dynamics. My question concerns bullet 3 in Sec 5.2, where the authors try to explain how Faber-Jackson Relation can be ...
1 vote
0 answers
121 views

Determining Time Based on Arc Seconds

So our arc day starts at 20°41'32 which is midnight (0:00) and ends 24 hours later at 21°42'42. According to my calculations it traveled 0 degrees, 59 minutes, and 30 seconds or 3570 arc seconds in 24 ...
1 vote
0 answers
39 views

How to get from SED to mag [AB]?

NGC 5406 has the following mag in SIMBAD g (AB) 13.104, r (AB) 12.215, i (AB) 11.803 I wrote a little python snippet to fetch the spectrum of NGC 5406 and compute the mags, but I've hit a wall. I'm ...
0 votes
0 answers
66 views

Flux from the Sun on the Earth using the Stefan-Boltzmann law

What is wrong with this computation, plase? I am getting the result of 4291.65 W m^{-2} instead of 1361 W m^{-2}. Thank you very much ...
0 votes
0 answers
46 views

Consistent values for density of galaxies between degree squared and steradian

I have a table of densities of galaxies : Expected number density of galaxies for photometric survey per unit area and redshift intervals, $\mathrm{d} N / \mathrm{d} \Omega \mathrm{d} z\left[\mathrm{...

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