Just to be clear:BillT wrote:
Actually Gaia can resolve some stars in the LMC.
Gaia has just completed its' first year of normal operation and one of the things mentioned in the ESA's blog post is this:
"Gaia has delivered detailed light curves for dozens of RR Lyrae type variable stars in the LMC, and the fine details revealed in them testify to the very high quality of the data."
They also posted their first HR diagram of just 2 million stars. They are saying that they will have the first major data release after the second year of operation is completed next year. The link is http://sci.esa.int/gaia/56387-gaia-s-fi ... ervations/
Hubble's angular resolution is ~0.05 arcsecond or ~2,500 AU at LMC distances (~50,000 pc).
The largest known star is red hypergiant VY Canis Majoris (VY CMa) with a diameter of 13.2 AU.
Hubble's resolution of ~60 AU at VY CMa's distance of 1,170 pc
means that it can't really even resolve this Milky Way hypergiant.
However, what Hubble & Gaia can do is to isolate stars from their neighbors for
discrete analysis including locating the centers of their blurry light signatures to very high accuracy.