Brian Jackson Assistant Professor of Physics at Boise State University

Assistant Professor of Physics at Boise State University

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This web page astrojack.com presently has an average traffic classification of zero (the lower the higher page views). We have scanned twenty pages inside the web site astrojack.com and found zero websites linking to astrojack.com. There are two contacts and locations for astrojack.com to help you reach them. There are three public web platforms retained by astrojack.com. This web page astrojack.com has been online for five hundred and seventy-one weeks, fourteen days, thirteen hours, and fourteen minutes.
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ASTROJACK.COM HISTORY

This web page astrojack.com was first documented on July 17, 2013. This site was last updated on December 13, 2013. This web page will go back on the market on the date of July 17, 2015. It is now five hundred and seventy-one weeks, fourteen days, thirteen hours, and fourteen minutes old.
REGISTERED
July
2013
UPDATED
December
2013
EXPIRED
July
2015

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A HAPPY DREAMHOST CUSTOMER

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417 ASSOCIATED RD #324 C/O ASTROJACK.COM

BREA, CA, 92821

US

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PAGE TITLE

Brian Jackson Assistant Professor of Physics at Boise State University

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Assistant Professor of Physics at Boise State University

CONTENT

This web page states the following, "Assistant Professor of Physics at Boise State University." We saw that the web site also stated " The Short Period Planets Group SuPerPiG." It also said " The Solar System Turns Out To Be A Little Weird Again. On March 10, 2018. Figure 1 The number of planets per star as a function of the planet-star mass ratio as discovered by Kepler. Dark and light blue curves are for stars less massive than the Sun, while the pink curve is for more massive stars. In their paper, Prof."

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Perigee is the point in an objects orbit around the earth where it is closest to the earth. Contrast with apogee, which is the point where the object is farthest from the earth. Should only apply to objects, such as the moon, which have elliptical orbits. The more elliptical the orbit, the greater the difference in distance at perigee and apogee. The eccentricity of an orbit is the degree to which the orbit is elliptical.