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Questions tagged [frame-of-reference]

For questions regarding the frame of reference of an observer in an astronomical situation.

0 votes
0 answers
74 views

I am a student studying HI HVC clouds, and I need to compare results from several HI surveys. I ran into a problem of "How to convert HIPASS barycentric velocities to LSRK velocities". ...
Firestar-Reimu's user avatar
0 votes
1 answer
97 views

Why does this code, using astropy LSR, give the same result in RV despite differing proper motions, i.e. 8.2802 km/s? I would expect that a change in proper motion should have an influence in the ...
Anna-Kat's user avatar
  • 559
1 vote
0 answers
55 views

The Geocentric Celestial Reference System (GCRS) and the International Terrestrial Reference System (ITRS) are based on an approximate Schwarzschild metric, as discussed for instance in Soffel & ...
pglpm's user avatar
  • 203
0 votes
0 answers
299 views

I want to convert some Cartesian vectors between the Geocentric Celestial Reference Frame (GCRF) and Earth-centered J2000 frame. I know that these two frames are nearly identical and, for most ...
NeutronStar's user avatar
  • 2,761
-1 votes
1 answer
231 views

If CMB redshift tells us our cosmological time dilation and we have two inertial observers in relative motion, who measure slightly different CMB redshift at the direction of their motion relative to ...
user avatar
7 votes
1 answer
276 views

I'm working on a mock image of a picture taken from a satellite (like ISS). Lets say I have a camera on ISS pointing in the direction of velocity (I have this velocity vector defined in ITRF and ...
jlipinski's user avatar
  • 329
7 votes
2 answers
1k views

The International Celestial Reference System (ICRS) defines coordinate axes that are closely aligned with those of the J2000 (aka EME2000) reference frame. The International Celestial Reference Frame (...
Cort Ammon's user avatar
1 vote
0 answers
39 views

The equation of motions due to the dipole magnetic force of a planet in a frame corotating with the planet and origin at the centre of planet assumed to be sphere components wise are given as below: \...
Lunthang Peter's user avatar
2 votes
1 answer
611 views

I have TEME coordinates from sgp4 propagation. I can convert those (in python) to ITRF given date and time of observation. How to convert coordinates from one of those two frames to horizontal azimuth ...
jlipinski's user avatar
  • 329
3 votes
3 answers
243 views

I have a polynomial model that can transform pixel X,Y coordinates to standard $\xi, \eta$. This model looks like this: $\xi/\eta = a_1 + a_2x + a_3y + a_4x^2 + a_5xy + a_6y^2 + a_7x^3 + a_8x^2y+a_9xy^...
jlipinski's user avatar
  • 329
4 votes
2 answers
2k views

UTC typically ticks with TAI. But to keep UTC from drifting far from the rotation angle of the Earth we occasionally add leap seconds to ensure that UTC does not drift too far from the UT1 timescale. ...
Jagerber48's user avatar
0 votes
0 answers
93 views

At the Wikipedia about an aberration, there is the phrase: a recommended galactocentric aberration constant of 5.8 µas/yr What is the galactocentric aberration? How is it calculated correctly? An ...
Imyaf's user avatar
  • 339
8 votes
2 answers
995 views

I am developing an n-body simulation software which simulates collisions. Most of these have a stationary frame of reference, meaning that orbiting objects may eventually move off the screen. To ...
WarpPrime's user avatar
  • 6,892
2 votes
0 answers
80 views

Last night in Greenville MI at around 9:15pm-9:25pm (I don't know the exact time) I saw what appeared to be a satellite appear and disappear and then a few seconds later another possible satellite ...
Michael's user avatar
  • 31
2 votes
2 answers
583 views

It is often stated that, "Planetary aberration is a combined result of the observer's motion and the time taken for light to travel from a body in the Solar System to the observer". I am not ...
JKrsl's user avatar
  • 121

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