What Is the Evening Star and Why Is It Not a Star?

The term “Evening Star” refers to the brightest celestial body visible in the western sky shortly after the Sun has set. Despite its traditional name, this luminous object is not a star—a massive, self-luminous ball of plasma—but a planet that shines only by reflecting the Sun’s light. This misnomer has persisted for millennia, yet its brilliance makes it the third brightest natural sight in the sky, surpassed only by the Sun and the Moon.

Identifying the Evening Star

The celestial object most frequently identified as the Evening Star is the planet Venus. Its overwhelming brightness far surpasses that of any true star in the night sky, often shining with an astronomical magnitude between -3.9 and -4.6, which makes it visible even in bright daylight under the right conditions. This intense luminosity is a result of a combination of factors related to the planet’s physical properties and its orbital position.

Venus is the most reflective planet in the solar system, a quality measured by its albedo. The planet’s dense, thick atmosphere, covered in highly reflective clouds of sulfuric acid, scatters and reflects about 70 to 84% of the sunlight that strikes it. This high reflectivity is coupled with Venus’s relative proximity to Earth; at its closest, the planet can come within approximately 41 million kilometers of our world, closer than any other planet.

Observing the Evening Star helps distinguish it from true stars because of its steady, silvery light. Unlike distant stars, which appear as point sources of light and seem to twinkle due to the distortion caused by Earth’s atmosphere, Venus presents a small visible disk. This larger apparent size means its light is less easily disrupted by atmospheric turbulence, resulting in a distinct, unwavering glow.

The Ancient Misnomer and Cultural Context

The name “Evening Star” originates from a time when ancient observers lacked the tools to distinguish between stars and planets. To the naked eye, the planet appears as a bright, wandering star, leading to its classification with the fixed stars. The same bright object seen in the morning and evening was often thought to be two separate celestial bodies.

The Greeks referred to the object seen after sunset as Hesperos, meaning “the star of the evening.” Conversely, the same object, when visible before sunrise, was called Phosphoros, or “the bringer of light,” which is the origin of the Roman name Lucifer. It was not until the 5th century B.C. that the Greek philosopher Pythagoras is credited with realizing the two bright objects were, in fact, one and the same planet.

This historical confusion, where a single planet was cataloged as two different “stars” depending on its appearance time, established the enduring tradition. The cultural significance of the Evening Star is profound, often symbolizing beauty, guidance, or protection in various mythologies and literature, such as the Roman goddess Venus, for whom the planet is named.

Understanding Its Visibility Cycle

The appearance of Venus as the Evening Star is directly governed by its orbit, which lies entirely inside Earth’s path around the Sun. Because of this inner orbit, Venus is classified as an inferior planet, and it never appears more than about 47 degrees away from the Sun in our sky. This constraint means the planet can only be seen low in the western sky after sunset or low in the eastern sky before sunrise.

The Evening Star phase occurs when Venus is on the far side of its orbit from the Sun, moving toward its greatest angular separation, known as greatest eastern elongation. At this point, the planet sets hours after the Sun, becoming a prominent beacon in the twilight sky. As it continues its orbit toward Earth, it appears to move closer to the Sun in the sky, eventually disappearing into the solar glare entirely.

The planet then transitions to its “Morning Star” phase after passing between Earth and the Sun, a position called inferior conjunction. It reappears in the predawn sky, marking its greatest western elongation as it moves away from the Sun. The complete cycle of shifting from Evening Star to Morning Star and back, known as the synodic period, takes approximately 584 Earth days.