The faster an object is receding, the more its light is shifted toward the red end of the spectrum.

And because the entire universe is expanding more or less uniformly, the faster an object is receding, the farther away it is.

The objects generally approach or (more usually observed) recede from the small region of their activity at high speed and high inclination.

The objects reportedly disappeared or receded when they were chased, but then suddenly reappeared when they started leaving.

At a distance, the individual objects recede into a mass of interlocking shapes and colors, elevating form over content.

The greater the velocity at which an object is receding in an expanding universe the greater its red shift.

And the greater the red shift, the farther away it is, because objects in the universe are receding at a velocity directly proportional to their distance.

If the object is receding from us, the lines shift toward the red.

One-point perspective where objects facing the viewer are orthogonal, and receding lines converge to a single vanishing point.

Distant objects receded into near invisibility: height meant nothing.