J002E3
en.wikipedia.org
en.wikipedia.org
I know this is a really old thing but the idea that we can determine composition of the surface of an object from so far away simply by looking at the light it reflects is absolutely incredible to me. Very science fiction. :)
And more generally spectroscopy: http://en.wikipedia.org/wiki/Spectroscopy
When people talk about Hubble (the guy, not the telescope) detecting the expansion of the universe by looking at redshift from distant galaxies, what he was actually looking at were spectral signatures. He saw all the patterns he expected to see from burning stars, but the lines were smeared out. Because he knew the patterns always form a consistent picture of the atomic structure, and he understood the doppler effect, he was able to estimate the distances of those objects quite accurately. Amazing stuff.
Noting that all the doppler shifts of other galaxies are red-shifts tells us that all the galaxies are moving away from us, but it still doesn't tell us whether speed correlates to distance in any way.
Figuring out the distance of galaxies is a different matter entirely, and is done with standard candles[0].
It's from the standard candles that we can measure distance, and only once we know the distance that way can we make a correlation between speed and distance, from which we see that the further away a galaxy is, the faster it is receding.
Only once we have found that there is a speed/distance curve can we estimate the distance to an object based on its doppler shift. We can't get it from the doppler shift alone.
[0] http://en.wikipedia.org/wiki/Cosmic_distance_ladder#Standard...
https://www.e-education.psu.edu/astro801/content/l4_p7.html
Hyperfine splitting of spectral lines in hydrogen gas caused by the interaction between electron and neutron spin allows you to map the hydrogen in our local Galaxy.
http://hyperphysics.phy-astr.gsu.edu/hbase/quantum/h21.html
As parent post says this is pretty standard astrophysics, just find any reasonable text in your local library. Or just Google 'astronomy .pdf' for a huge range of handbooks and presentations.
J002E3 - piece of Apollo 12 returned
to Earth orbit after 31 years
That was much, much more useful and informative.To avoid an onslaught of HN traffic to the telnet server, I will just say to go to ssd.jpl.nasa.gov, and click through to find it. Once you're telnetted in, enter J002E3.
But according to the Apollo 12 wikipedia page: "a small error in the state vector in the Saturn's guidance system caused the S-IVB to fly past the Moon at too high an altitude to achieve Earth escape velocity".
Isn't this just a fancy way of saying that it was white?
"Some compounds, like titanium oxide, only appear in the spectra of very cool stars." [1]
Obviously this wasn't a star, so it must be a manmade object.
[1] From http://skyserver.sdss.org/dr1/en/proj/advanced/spectraltypes...