I just had a nice chat with one of the security guards and she told me to stay safe with a smile on her face. That's the second surprise I've had today.
I drove by a group of people in a small Texas town with protest signs. I never thought that would've happened, but I've been proven wrong. It'll be my turn in a bit.
That's some serious stuff. I wouldn't fully trust that guy if I were you, so be prepared for the worst if you're seriously committed to this. If not, I'd find a way out, if possible.
It is commonly believed that our own Milky Way is on a collision course with
the neighbouring Andromeda galaxy. As a result of their merger, predicted
in around 5 billion years, the two large spiral galaxies that define the present
Local Group would form a new elliptical galaxy. Here we consider the latest
and most accurate observations by the Gaia and Hubble space telescopes,
along with recent consensus mass estimates, to derive possible future
scenarios and identify the main sources of uncertainty in the evolution
of the Local Group over the next 10 billion years. We found that the next
most massive Local Group member galaxies—namely, M33 and the Large
Magellanic Cloud—distinctly and radically affect the Milky Way–Andromeda
orbit. Although including M33 increases the merger probability, the orbit
of the Large Magellanic Cloud runs perpendicular to the Milky Way–
Andromeda orbit and makes their merger less probable. In the full system,
we found that uncertainties in the present positions, motions and masses of
all galaxies leave room for drastically different outcomes and a probability of
close to 50% that there will be no Milky Way–Andromeda merger during the
next 10 billion years. Based on the best available data, the fate of our Galaxy
is still completely open.
Till Sawala, Jehanne Delhomelle, Alis J. Deason, Carlos S. Frenk, Jenni Häkkinen, Peter H. Johansson, Atte Keitaanranta, Alexander Rawlings & Ruby Wright
South Padre Island