'WeВ Don'tВ Planet'В Episode 5: The Hertzsprung-Russell Diagram

By Paul Sutter, Astrophysicist | May 26, 2017 07:30am ET
If you sampled the hundreds of billions of stars in any galaxy and plotted their luminosity (their brightness measured from a fixed distance - so, in other words, their "true" brightness) and their color, you might expect the points to be essentially scattered around randomly.
But the work of Ejnar Hertzsprung and Henry Russell around 1910 revealed
something much more surprising: almost all stars landed within a thin diagonal band stretching from bright-and-blue to dim-and-red, with an odd clump of dim-and-blue and an almost horizontal branch of bright-and-red.
After decades of research, we now realize that the features on the Hertzsprung-Russell diagram reveal the evolutionary path of stars as they are born, age, and die.
The thin diagonal band is now known as the Main Sequence, and all stars fusing hydrogen in their cores lay along it. When stars first ignite with fusion, they land somewhere along that sequence, depending on their initial mass. As they age, stars slowly become brighter and blue, creeping up and left on the diagram.
After exhausting their supply of available hydrogen at the ends of their lives, stars leave the Main Sequence, inflating to become red giants - this is the horizontal branch.
Finally, after millions of years of paroxysms and chaotic outflows ending in the formation of a planetary nebula, only the unburnt core of carbon and oxygen survives - the white dwarfs, situated in the dim-and-blue corner of the diagram.
Thus the Hertzsprung-Russell diagram is a complete life history of a star: Once we know the current age of a star and its location on the diagram, we can accurately predict its fate over the course of billions of years.
"We Don't Planet" is hosted by Ohio State University astrophysicist and COSI chief scientist Paul Sutterwith undergraduate student Anna Voelker. Produced by Doug Dangler, ASC Technology Services. Supported by The Ohio State University Department of Astronomy and Center for Cosmology and AstroParticle Physics. You can follow Paul on Twitter and Facebook.
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Author Bio
Paul Sutter, Astrophysicist
Paul Sutter is an astrophysicist at The Ohio State University and the Chief Scientist at COSI Science Center. Paul received his PhD in Physics from the University of Illinois at Urbana-Champaign in 2011, and spent three years at the Paris Institute of Astrophysics, followed by a research fellowship in Trieste, Italy, His research focuses on many diverse topics, from the emptiest regions of the universe, to the earliest moments of the Big Bang, to the hunt for the first stars.
As an "Agent to the Stars," Paul has passionately engaged the public in science outreach for several years. He is the host of the popular "Ask a Spaceman!" podcast, where he answers questions posted on social media. In addition, Paul writes for Space.com, regularly appears at events and in the media, and consults for film and TV productions. Paul Sutter, Astrophysicist on