Distant Worlds: What We Know About Extra-Solar Planets And Their Potential For Habitability

Greetings, fellow astrophiles!

I’m pleased to announce that CNYO is co-sponsoring a lecture with the Cazenovia College Science Cafe Committee on one of the great achievements in observational astronomy in the last decade – the discovery and characterization of extra-solar planets (exoplanets). If so inclined, feel free to RSVP on our meetup.com event page. Details below:

Distant Worlds: What We Know About Extra-Solar Planets
And Their Potential For Habitability

Speaker: Dr. Leslie Hebb, Hobart and William Smith Colleges

Date: March 1, 2017

Time: 6:30 to 8:00 pm

Parking: Free on campus after 6:00 p.m., available on Lincklaen, Seminary, Sullivan, and Nickerson Streets

Location: Morgan Room, basement of Hubbard Hall, Cazenovia College

Since the first extra-solar planet was discovered around the star 51 Pegasi, there has been an explosion of research aimed at discovering and characterizing planets around other stars. With the launch of NASA’s Kepler mission, the number of known exoplanets has grown to nearly 5000 including almost 500 multi-planet “solar systems”. Through these and other discoveries, we have learned that exoplanets are ubiquitous throughout the Galaxy, and many planetary systems look very different than our own Solar System. This research has radically transformed our thinking about how our own Solar System in particular and solar systems in general form and evolve. I will discuss how exoplanets are detected and characterized, the current exoplanet census, and our current understanding of how planetary systems form and evolve. I will also discuss how we identify potentially habitable worlds and what future missions are designed to identify and characterize habitability.

One Thought on “Distant Worlds: What We Know About Extra-Solar Planets And Their Potential For Habitability

  1. Pingback: “Upstate NY Stargazing In March” Article Posted To newyorkupstate.com And syracuse.com | CNY Observers & Observing

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