mas\text{mas}

milliarcsecond

Angleexact by definition

The milliarcsecond is a thousandth of an arcsecond, about 4.848 × 10⁻⁹ radians. It is the working unit of modern astrometry: a parallax of 1 mas corresponds to a distance of one kiloparsec, and the Gaia mission measures positions and parallaxes at this level for over a billion stars.

Watch out: Very long baseline interferometry and Gaia both produce angles this small, but they are measuring different things. A parallax in mas inverts to a distance; a proper motion in mas per year is a transverse velocity that also needs the distance before it means anything in kilometres per second.

1 mas\text{mas} 2.7777778e-07 ∘^{\circ}

One milliarcsecond in every angle unit

1,000microarcsecond (μas)
1milliarcsecond (mas)this unit
0.00484814microradian (μrad)
0.001arcsecond (″)
0.0000166667arcminute (′)
0.00000493827mil (NATO) (mil)
0.00000484814milliradian (mrad)
3.08642e-07gradian (gon)
2.77778e-07degree (°)
2.46914e-08compass point (point)
1.85185e-08hour angle (h)
4.84814e-09radian (rad)
3.08642e-09quadrant (quad)
7.71605e-10revolution (rev)