Today I was rewriting a talk I've been giving lately about a peculiar class of planets known as "hot Jupiters": gas giant planets with period of only a few days. In past talks I would say that based on the example of our Solar System---with its giant planets in very wide, long-period orbits---"no one could have expected these hot, close-in Jupiters!" Well, this isn't entirely true. There was a person who predicted the existence of hot Jupiters well before the first exoplanet was found around a normal star in 1995. I wanted to change my introduction to give proper credit where it is due, but I couldn't remember the intrepid astronomer who made this bold prediction. So I sent an email to Geoff Marcy: On Apr 28, 2010, at 2:34 PM, John Johnson wrote: Hi Geoff, I recall you mentioning an old paper from the 60's in which the author noted that there was no reason not to expect Jupiters in few-day orbits. Can you point me to that paper or remind me of ...
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