dotancohen said:
That page makes the distinction between the Sun's movement in the galaxy and the Sun's movement in the Local Standard of Rest. That is interesting, and makes me wonder in which direction is the entire galaxy moving? Is it in the direction of Andromeda, as I know that we will collide with Andromeda some day, or will we meet Andromeda in some other location in the sky?
I know that there is no origin in space from which to derive a direction of movement, so the question of in which direction is the Milky Way traveling might not even be relevant. I suppose that if I had to pick a reference frame I would pick the distant galaxies as an envelope and consider the Milky Way's movement inside that envelope. Or is that also impossible, seeing how those distant galaxies are apparently moving away from us?
The "solar apex" is not quite the direction you were asking for. That is a slight motion of the sun relative to its immediate neighborhood. It is only some 16-20 km/s.
You were asking about the direction the sun is heading in its orbital motion around the galactic center---about 220-250 km/s.
The direction of that orbital motion (which we share with the surrounding crowd of stars except for minor deviations) can be calculated by finding a direction which is perpendicular to the direction of galactic center and also perpendicular to the galactic north pole.
Our general orbital direction is therefore about 21 hours (RA) and 48 degrees celestial "North latitude".
I would say that our direction is more or less towards the star DENEB in the constellation CYGNUS. I could be wrong but you probably can check easily. Please tell me if I am way off.
That is not the star Vega. A lot of internet sources seem to think it is the direction of Vega, or the constellation Hercules. I think they've confused it with the Solar Apex (our drift within the overall motion of our neighbors).
Here is a source:
==quote==
Below we give some data for the Galactic Center (this and all following positions for epoch 2000.0):
Right ascension 17 : 45.6 (h : m)
Declination -28 : 56 (deg : m)
Distance 28 (kly) The Galactic North Pole is at
Right ascension 12 : 51.4 (h : m)
Declination +27 : 07 (deg : m)
The coordinate data given here were extracted from the online coordinate calculator at Nasa/IPAC's Extragalactical Database (NED) (also available by telnet).
Our Sun, together with the whole Solar System, is orbiting the Galactic Center at the distance given, on a nearly circular orbit. We are moving at about 250 km/sec, and need about 220 million years to complete one orbit (so the Solar System has orbited the Galactic Center about 20 to 21 times since its formation about 4.6 billion years ago).
In addition to the overall Galactic Rotation, the solar system is moving between the neighboring stars (peculiar motion) at a velocity of about 20 km/s, to a direction called "Solar Apex," at the approximate position RA=18:01, Dec=+26 (2000.0); this motion has been discovered by William Herschel in 1783.
Considering the sense of rotation, the Galaxy, at the Sun's position, is rotating toward the direction of
Right Ascension 21:12.0, Declination +48:19. This shows that it rotates "backward" in the Galactic coordinate system, i.e. the Galactic North Pole is actually a physical South Pole with respect to galactic rotation (defined by the direction of the angular momentum vector).
==endquote==
http://seds.org/messier/more/mw.html