Apologies for the confusing title, it is late here. I'm wondering exactly what meaning the "time coordinate" has in General Relativity. We always write the line element as ds2=g00(dx0)2+2g0idx0dxi+gijdxidxj,
Answer
Let (Mn+1,g) be a Lorentzian manifold. Given p∈M, we will show that there is a coordinate system (xμ) defined on an open set p∈U⊂M such that ∂0 is a timelike vector field, and ∂i are spacelike vector fields for i=1,…,n.
Let (xμ) be an arbitrary chart defined on U∋p. It is known that TpM is the span of {∂0,∂1,…,∂n}. As gp has signature (−,+,…,+), we may find linearly independent vectors vμ, μ=0,1,…,n, such that gp(v0,v0)=−1, gp(vi,vi)=+1. These vectors are linear combinations of {∂0,∂1,…,∂n}. By a linear change of coordinates, we can find a coordinate system (yμ) such that ∂/∂yμ=∂′μ=vμ at p. By continuity, there is a neighborhood V0⊂U of p such that g(∂′0,∂′0)<0, i.e., ∂′0 is timelike on V0. Similarly, there exist neighborhoods Vi such that g(∂′i,∂′i)>0 on Vi. We take V=V0∩⋯∩Vn, which is a neighborhood of p. By changing each coordinate value by a constant, we can adjust the origin without changing the aforementioned vector fields. Then (yμ) is the desired coordinate system on V.
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