Detailed 3D map of Milky Way shows 'warped' shape
theguardian.com
theguardian.com
One thing that seems to have changed is visible satellites. Or maybe I am just missing them. I recall as a child watching the sky with my grandfather and you'd regularly see a "star" moving across the sky and he'd excitedly point it out as a satellite.
You can build an arduino-powered "barn-door tracker" for ~$40 that will significantly help with this. https://www.youtube.com/watch?v=5hqXqqTtWzU
If you're hoping to hook up a DSLR to a telescope this won't help though, not big enough. Plus, this style of tracker only tracks through one axis, limiting exposure time to ~10seconds before stuff gets blurry & drift destroys the image... but that's still better than the ~2seconds or so that you get without it.
*Found it: https://science.nasa.gov/science-news/science-at-nasa/2003/2...
[0] https://hitchhikers.fandom.com/wiki/Total_Perspective_Vortex
Edit: For this purpose, I think that this "Chrome Experiment"[2], might be better.
Also see "Gaia Sky"[3] which I haven't tried, but which looks really interesting and may well do what you want.
[1] https://en.wikipedia.org/wiki/Celestia
[2] https://experiments.withgoogle.com/100000-stars
[3] http://sci.esa.int/gaia/60036-gaia-data-release-2-virtual-re...
> The Polish team also found younger Cepheids lie nearer the centre of the Milky Way, while older Cepheids are further out. A computer simulation revealed there would need to have been star-forming events 64m, 113m and 175m years ago to produce the distribution of Cepheids seen today.
I don't get why the Cepheids are bunched. Even with the modeling video. It shows them forming in bursts, yes. And with differential rotation, they bunch on one side. But still, it shows the formation bursts mainly on one side.
So why?
"The stars and gas in the Milky Way rotate about its center differentially, meaning that the rotation period varies with location. As is typical for spiral galaxies, the orbital speed of most stars in the Milky Way does not depend strongly on their distance from the center. Away from the central bulge or outer rim, the typical stellar orbital speed is between 210 ± 10 km/s (470,000 ± 22,000 mph). Hence the orbital period of the typical star is directly proportional only to the length of the path traveled."
If the earth was on the other side of the galaxy the group would appear there because the stars we would find would be there. I think the article writer misunderstood the astronomer about this and mismatched responses.
Edit: https://m.media-amazon.com/images/I/61IdlF0D2eL._AC_UL320_.j...