Students

This page will contain the names of all of the students in our classes. Please use this page to help coordinate collaboration between you and other students in the course. The list below reflects the rosters at the start of school but may change as the drop/add period continues.

Period 1

Anthony Abron
Thomas Allen
Brian Beck
Billy Bevivino
Chris Bonner
Jack Connor
Timmy Dagit
Matt Jones
Will Ka
Britt Kershne
Alex McLaughlin
John Nassib
Ross Sherman
Colin Sullivan
David Van Sleet
Nick Wells

Period 2

Drew Barrar
Richard Chakejian
JP Clark
Joe Dolan
Jonathan Dollfus
Colin Hayes
John Heller
Ryan Hilburn
Sam Leinhauser
Matthew Maul
Billy McCullough
Kevin McKnight
Connor McNeill
Luke McStravick
Nick Melchiorre
Mark Palmarella
Andy Pancoast
Matthew Ramirez
Jonathan Rava
Jack St. Amour, II
Hadid Thomas
Ricky Walsh

Period 5

Kevin Burns
Justin Coyle
Marc D'Angelo
Erik Dresden
Nicholas Flowers
Troy Gallen
Tony Gruenling
Bryce Jablonski
Pat Lewer
Ryan Mansfield
David Monzo
Murphy Rogers
Tripp Traynor
Michael Vermeil
Jay Zazzera

2 comments:

  1. When small stars die they will form red giants first and Earth will go through a fiery death. Then, the small star will form a planetary nebula. Lastly, the cooled down carbon mass will form a white dwarf. Large suns sometimes have enough energy to fuse helium after the hydrogen. In this case they will have a much longer life span. These stars have the potential to form black holes after they finally die off.

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  2. A black body is an object that absorbs 100 percent of all electromagnetic radiation (that is, light, radio waves and so on) that falls on it. A common image here is that of a brick oven with the interior painted black and the only opening a small window. All light that shines through the window is absorbed by the interior of the oven and none is reflected outside the oven. It is a perfect absorber. As it turns out, this definition of being perfect absorbers suits stars very well! However, this just says that a blackbody absorbs all the radiant energy that hits it, but does not forbid it from re-emitting the energy. In the case of a star, it absorbs all radiation that falls on it, but it also radiates back into space much more than it absorbs. Thus a star is a black body that glows with great brilliance! (An even more perfect black body is a black hole, but of course, it appears truly black, and radiates no light.)

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