[HN Gopher] The New Story of the Milky Way's Surprisingly Turbul...
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The New Story of the Milky Way's Surprisingly Turbulent Past
Author : pseudolus
Score : 22 points
Date : 2024-01-28 12:28 UTC (2 days ago)
(HTM) web link (www.scientificamerican.com)
(TXT) w3m dump (www.scientificamerican.com)
| morphle wrote:
| https://archive.ph/DOK5W
| chasil wrote:
| "Astronomers are making the first exact maps of the Milky Way:
| locations of stars in three dimensions..."
|
| I thought that "standard candles" were required to estimate the
| distance to any region of space?
|
| How can the distance to arbitrary stars be determined without
| these markers?
| thatswrong0 wrote:
| Gaia is orbiting around the L2 Lagrange point. As it traverses
| its orbit, the stars will appear to wiggle (relative to their
| previous recorded position) because of the stellar parallax
| effect. This (along with precisely knowing Gaia's orbit)
| enables scientists to accurately measure the distance to the
| star - if it wiggles more, it's closer. If it wiggles less,
| it's further away.
|
| There is a limit to this method of measurement, based on the
| accuracy of the telescope. For Gaia:
|
| > The European Space Agency's Gaia mission is expected to
| measure parallax angles to an accuracy of 10 microarcseconds
| for all moderately bright stars, thus mapping nearby stars (and
| potentially planets) up to a distance of tens of thousands of
| light-years from Earth.
|
| The Milky Way is about 100,000 light-years wide. So it is able
| to accurately measure the distance for a _lot_ of stars around
| us in our galaxy.
|
| This video probably explains it better:
| https://www.youtube.com/watch?v=Jdy09y0A4t0
| vikingerik wrote:
| To be clear (and the video isn't), the parallax is observed
| and calculated mostly from the diameter of Earth's orbit,
| with observations made six months apart. Gaia's L2 orbit is a
| much smaller factor, on the order of 1M km compared to
| Earth's orbital diameter of 300M km.
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