Venus Shines at Its Most Brilliant This Week: How to See It

Venus, February 2014
Venus reaches its point of greatest brilliancy on February 15 when its increasing distance and the broadening width of its crescent reach an optimum combination. (Image credit: Starry Night Software)

Venus will perform a balancing act this week.

Normally Venus, like most objects in space, gets fainter as it gets farther away from Earth. However, as Venus moves around the sun, it is lit from different angles, and this also affects its brightness.

This week, the planet's distance from Earth and its angle to the sun combine so that Venus shows more of its reflective surface than at any other point in the sun's orbit, causing the planet to shine at its very brightest. Unfortunately, observers can only see Venus at its brightest by getting up early in the morning. Its current location just west of the sun makes it a "morning star" rising two hours before the sun. [See amazing night sky photos taken by stargazers in February 2014]

Ptolemy declared the 20 brightest stars in the sky to be "of the first magnitude," and the faintest stars he could see to be "of the sixth magnitude." Once he established these two end points for his scale, he could assign the stars of intervening brightness to the various steps on the scale.

In 1856, British astronomer Norman Robert Pogson attempted to apply modern mathematics to Ptolemy’s scale. He noticed that first magnitude stars were almost exactly 100 times brighter than sixth magnitude stars, and used that to establish a logarithmic relationship between star brightnesses. The main problem was what to do with objects that were brighter than first magnitude. Pogson extended the scale "upwards" from 1st magnitude to 0 magnitude, minus 1 magnitude, and beyond.

On Pogson’s scale the brightest star, Sirius, comes in at magnitude minus 1.44, the full moon at minus 12.7, and the sun at minus 26.75.

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Geoff Gaherty
Starry Night Sky Columnist

Geoff Gaherty was Space.com's Night Sky columnist and in partnership with Starry Night software and a dedicated amateur astronomer who sought to share the wonders of the night sky with the world. Based in Canada, Geoff studied mathematics and physics at McGill University and earned a Ph.D. in anthropology from the University of Toronto, all while pursuing a passion for the night sky and serving as an astronomy communicator. He credited a partial solar eclipse observed in 1946 (at age 5) and his 1957 sighting of the Comet Arend-Roland as a teenager for sparking his interest in amateur astronomy. In 2008, Geoff won the Chant Medal from the Royal Astronomical Society of Canada, an award given to a Canadian amateur astronomer in recognition of their lifetime achievements. Sadly, Geoff passed away July 7, 2016 due to complications from a kidney transplant, but his legacy continues at Starry Night.