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1 vote
1 answer
36 views

Determining star position and velocity to deduce closest approach?

I am trying to replicate the results found for Gliese 710's closest approach of ~0.05 parsecs in 1.3 million years approximately. I thought that by plotting the sun at (0,0) and using the stars ra,dec,...
user2279603's user avatar
3 votes
1 answer
67 views

Modelling a fully relativistic White Dwarf Star

I am trying to model a fully relativistic white dwarf using different central densities. Using the below equations: $\frac{dP}{dm} = -\frac{Gm}{4\pi r^4}$ $\frac{dr}{dm} = -\frac{1}{4\pi\rho r^2}$ and ...
A.M's user avatar
  • 31
0 votes
0 answers
101 views

Galaxy S4G database: convert pixel to kpc

I am referring to S4G database (https://irsa.ipac.caltech.edu/data/SPITZER/S4G/overview.html ). The information on the length of galaxies, and various length parameters are given in terms of pixels. ...
Angela's user avatar
  • 1,023
1 vote
0 answers
64 views

What are astrocentric co-ordinates?

A program I am using requires the ecliptic astrocentric cartesian coordinates of the Earth and the Sun in AU however I have never come across these co-ordinates before and the internet doesn't provide ...
Jordan Allen's user avatar
4 votes
1 answer
205 views

Drawing night sky of planets other than Earth (invariable plane ambiguity)

I'm writing an application that draws maps of night sky that can be visible from other planets (ultimately they are to be exoplanets). Mostly I do it out of curiosity :). I's thinking a lot where I ...
Felix.leg's user avatar
  • 137
0 votes
1 answer
695 views

How do I convert a .FITS into a numpy array (or a file that can be used in Python)? [closed]

I'm trying to train an AI algorithm to determine photometric redshifts of galaxies, and to do so I have a .FITS file which contains the training data. I need to convert this .FITS file into a format ...
Lara's user avatar
  • 11
0 votes
2 answers
329 views

How to represent orbital velocity of a planet on an elliptical path in terms of time?

Before reading this long message, please know that this is question is posted to know whether there is a method to find the relation between between the orbital velocity of a planet on an elliptical ...
noob anomaly's user avatar
0 votes
0 answers
104 views

How can we calculate solar and lunar longitude in java?

I want to develop panchangam logically. So, I want to find solar longitude and lunar longitude. Could you please help me to find the solar and lunar longitudes in java or any mathematical formula for ...
Kalyan Dammu's user avatar
0 votes
0 answers
30 views

Lane-Emden. Quasi-linearization method

ow to prove this theorem? I have a doubt. Theroem: Suppose that $w(x,\alpha)$ solved $\ddot{w}+\frac{2}{x}\dot{w}+\alpha^{2}w=0$ with $w(0)=1$, $\dot{w}(0)=0$, $w(1)=0$. Then $v(x,\alpha) := \omega w(...
Adjo's user avatar
  • 1
0 votes
1 answer
170 views

Are the orbits in my simulation correct? [closed]

I'm creating a simulation of our solar system. I used data from https://nssdc.gsfc.nasa.gov/planetary/factsheet/ and I supplied the planets with perihelion and aphelion values. But I'm afraid the ...
Derk Jan Speelman's user avatar
2 votes
1 answer
314 views

Sidereal time calculation from orbital elements and mean anomaly

I'm following the instructions given here for calculating the apparent position of the planets in the sky and I've come to calculating the sidereal time in section 1.8. The formula for calculating ...
Mrfence's user avatar
  • 121
1 vote
0 answers
54 views

Cosmological parameters from a certain data set

Specifically, I need to find the cosmological parameters $Ω_i$ from a certain data set (with error bars) of redshift $z$ and luminosity distance $d_L$ using a Fisher Information matrix. I know that my ...
Renan Nobuyuki Hirayama's user avatar
1 vote
0 answers
63 views

Numerical error in implementation of universal variables [closed]

I am trying to implement (in Python for now) low thrust orbit propagation for spacecraft using universal variables. For a given central body with the gravitational parameter $\mu$ and an orbit with ...
Ganymed_'s user avatar
1 vote
1 answer
847 views

SDSS spectra FITS format: what do the rows mean?

This might be in the FITS Header, but I couldn't find it. I am looking at the FITS files for SDSS 1D spectro images from DR7 using the SDSS Data Archive Server at das.sdss.org (there might be an ...
ShanZhengYang's user avatar
2 votes
1 answer
2k views

Precession of Mercury (Python simulation)

I was trying to simulate the precession of Mercury based on the perturbed solution, and my questions about its implementation in python can be seen here: https://scicomp.stackexchange.com/questions/...
Sam's user avatar
  • 129

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