Venus, the planet nearest to the Sun, exhibits a full range of phases much like our Moon, from new to gibbous to full. The phase angle (the SunβVenusβEarth angle) determines how much of the sunlit side is visible from Earth, and this fraction is given by the simple cosine law of illumination.
The apparent angular size of Venus on the sky depends primarily on its physical radius and its instantaneous distance from Earth. Because Venus orbits inside Earthβs orbit, its distance varies between about 0.28β―AU at inferior conjunction and 1.72β―AU at superior conjunction, causing the observed disk to change dramatically in size.
Combining the geometry of the phase with the distance yields the observable illuminated diameter. The geometric angular diameter (ΞΈ) is calculated from the planetβs radius (R) and the EarthβVenus distance (d). The illuminated fraction (f) modifies the visible portion of that disk according to the phase angle (Ξ±).
How does Venus' phase change throughout its orbit?
What determines the apparent size of Venus in the sky?
How does the phase angle affect Venus' visibility?
Why does Venus never appear as a full disk from Earth?
Can you explain how Venus' distance affects its phase size?
How do I calculate the phase fraction of Venus?
What is the significance of Venus' phases in astronomy?
Results are for informational purposes only and do not constitute professional advice.
