Black Hole Apocalypse | Determining the Distance and Mass of Cygnus X-1

PBS Learning Media
Contributed By
PBS Learning Media
Resource Type
Classroom Material
Keywords
WGBH NOVA Black Hole Apocalypse Cygnus X-1 parallax cosmic distance Kepler's laws Kepler black hole astronomical measurements Mark Reid VLBA Very Long Baseline Array
Subjects
Science
Grade Levels
Grade 9 Grade 10 Grade 11 Grade 12
Related Resources

Black Hole Apocalypse | Determining the Distance and Mass of Cygnus X-1

Learn how astronomers used parallax to more accurately determine the distance to Cygnus X-1, a stellar black hole, in this video from NOVA: Black Hole Apocalypse. People perceive depth using the principle of parallax—our two eyes see the world from slightly different vantage points. To calculate the distance to a celestial object, astronomers use Earth’s orbit to provide two vantage points. Astronomers measured the tiny parallax angle of Cygnus X-1 using an array of 10 radio telescopes across the world. They then determined that Cygnus X-1 is about 6,000 light-years away and calculated its mass to be about 15 solar masses. This resource is part of the NOVA: Black Hole Apocalypse Collection.

Publisher
PBS Learning Media

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