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What Is Radiofrequency Energy (Rf)?

Radiofrequency (RF) energy is another name for radio waves. It is one form of electromagnetic energy that makes up the electromagnetic spectrum. Some of the other forms of energy in the electromagnetic spectrum are gamma rays, x-rays and light. Electromagnetic energy (or electromagnetic radiation) consists of waves of electric and magnetic energy ...

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WhatIsRadiofrequencyEnergy
Biology

Gray Wolf - Canis lupus

Historically, most Native Americans revered gray wolves, trying to emulate their cunning and hunting abilities. However, wolves became nearly extinct in the lower 48 states in the early part of the ... Continue reading

GrayWolfCanislupus
Astronomy

Near-Earth Supernovas

Supernovas near Earth are rare today, but during the Pliocene era of Australopithecus supernovas happened more often. Their source was an interstellar cloud called 'Sco-Cen' that was slowly gliding by ... Continue reading

Supernovas
Chemistry

What is Oxidation?

The term 'oxidation' derives from the ancient observation of rust (oxide) formation. Early chemists could determine an increase in the weight of a metal as it apparently captured something from the ... Continue reading

WhatisOxidation
Astronomy

Look, Up in the Sky. It's A Bird. No It's A Meteorite!

Most folks probably think of swallows and the ringing of the Mission bells when the words San Juan Capistrano are heard or seen. This is a popular tradition that celebrates the return of cliff ... Continue reading

MeteoriteSky

Light Fantastic

LightFantasticOn the next hot summer day, imagine what would happen if the Sun suddenly became one million times brighter. Ice cream would quickly melt, sunscreen lotion wouldn't work very well, and that's just the beginning. Thankfully, our Sun doesn't misbehave this way. Yet, in early 2002, we witnessed strange behavior by a star in the dim winter constellation Monoceros (Moh-NO-ser-os) the Unicorn. The star, named V838 Monocerotis (Moh-NO-ser-u-tis) or V 838 Mon for short, grew very bright then cooled and faded away. The glow was bright enough to light up layers of dust surrounding the star, like a flashlight shining through smoke in a dark room.

What caused this star to become the brightest star in our Milky Way Galaxy for a short time? Astronomers think V838 Mon suddenly grew hotter and swelled to nearly 1,000 times larger than our Sun. At that size, we could see much more of the star, which explains why V838 Mon appeared so much brighter. Just think...at that size, our Sun would swallow Earth and stretch all the way to Jupiter's orbit!

NASA's Hubble Space Telescope watched the dust shell around V838 Mon over many months after the outburst. Every time Hubble astronomers take a picture, the dust ring looks larger than before. But, in the Hubble pictures, the dust really isn't growing. Instead, light from the flash is sweeping through the dust, lighting up different parts. This illusion is called a 'light echo.'