Quick question to check I'm visualising this correctly:

 

Over the course of a day/night cycle, from any point on the Earth you actually see as much of the celestial sphere as you are ever going to during the year (ignoring precession of equinoxes etc).

 

The only thing that stops you seeing some stars is the inconvenience of the Sun; you have to wait for it to "move along" the ecliptic and stop blinding you with pesky daylight.

 

Is that correct?

Right. The earth's orientation with respect to the "fixed" stars does not change over the course of the year.

Thanks swansont.

Right. The earth's orientation with respect to the "fixed" stars does not change over the course of the year.

 

I thought that the tilt of the Earth affected what stars are visible at what times.

I thought that the tilt of the Earth affected what stars are visible at what times.

 

Yes and no. The orientation of the Earth's axis is nearly constant with respect to the fixed stars. Polaris is always in the same spot in the sky, day and night, summer and winter, and all stars (except the sun, of course) follow the same path across the sky (that is, concentric circles around Polaris) every sidereal day. What you actually get to see with the naked eye depends on the presence or absence of the sun, but that is affected by the Earth's tilt.