The linear distance from the galaxy center = -LSB-(2p × (distance to the galaxy) × (
angular distance in degrees)-RSB- / 360 °.
Not exact matches
By comparing the
angular differences
in those paths to the geographic
distances between the observers, astronomers could calculate Earth's
distance from Venus.
Another
distance cue, called
angular declination, relies on the vertical position of an object
in the visual field.
Remember way back
in the planetary science chapter that the linear
distance can be found from the
angular distance if you know the
distance to the object?
DS5: The construction of an engineering demonstrator low frequency array resembling our vision of an SKA station and exploration of the practical issues involved
in multi-beam acquisition and signal - processing concepts The operation of links
in SKADS (using the European research fibre network GÉANT) to join a number of SKADS multi-beaming demonstrators separated by
distances up to many hundreds of kilometres, to demonstrate the high
angular resolution imaging capabilities required by the SKA community.
When the signals of individual telescopes are combined using the interference of radio waves, this array of telescopes has the
angular resolution equivalent to a radio telescope of 350 000 km
in diameter — almost the
distance between the Earth and Moon.