Tuesday, January 31, 2012

The Birth of Planck's Constant




In the late 1900s, a German physicist named Max Planck (1858-1947) had discovered an empirical formula that fit the blackbody spectra, which is…

E = spectral radiance
C1 & C2 = constants
Lambda = wavelength
T = temperature in Kelvin

To evaluate the constants, Planck considered a cavity of temperature filled with blackbody radiation. (Can be thought as a hot oven filled with standing waves of electromagnetic radiation).  Planck attempts to extend the permitted wavelength forever to increasingly shorter wavelengths, such as 2L, L, 2L/3, etc.

 What is Planck’s dilemma if he attempts to extend the wavelengths?

Each permitted wavelength should and could only receive an amount of energy equation to kT, a direct similarity to ideal gas law. This is considered an “ultraviolet catastrophe” because the infinite number of infinitesimally short wavelengths implied that an unlimited amount of blackbody radiation energy was contained in the oven.





Planck attempts to circumvent this problem by using a clever mathematical trick that involves assuming that a standing electromagnetic wave of wavelength and frequency could not acquire just an arbitrary amount of energy, but instead the wave could have only specific energy values that were integral multiples of minimum wave energy, known as quantum of energy.  So given the assumption of quantized wave energy with a minimum energy proportion to the frequency of the wave, the ultraviolet catastrophe can be avoided.
Planck hopes that the constant "h" will be 0, hoping that an artificial constant should not remain as his result.
Planck stratagem worked, but his formula only worked if the constant “h” is a certain value.
Therefore,  the value became known as Planck’s constant, which is 6.26E-34 J/s.


Monday, January 23, 2012

Bright Stars + Physics = No Girlfriend



                                 

A conversation of me and my girlfriend a couple of years ago in Hawaii:
Me:  This night is perfect! (Trying to sneak a kiss)
My Girlfriend: Yes, it is the best!! (We kissed)
Me: You are the best kisser ever. (She laughs)
My Girlfriend: (Looking through the telescope) Wow, the stars really look bright tonight.
Me: Yes they sure are. That is called the Alpha Centauri. It’s almost impossible to see it from where we lived, but here we can see part of it.
My Girlfriend: Really? They are so bright… but it’s not brighter than the sun though.
Me: (I laugh) No honey, Alpha Centauri is actually brighter than the sun.
My Girlfriend: No I don’t believe you. It’s not like you can measure its brightness.
Me: Oh yes I can.

The brightness of any star is measured in terms of the radiant flux that the star emits. The radiant flux is the total amount of light energy of all wavelengths that crosses a unit area oriented perpendicular to the direction of the light’s travel in time.  The radiant flux also received and depends on the object luminosity, energy being emits per second, and also the distance being observe.

The equation to measure radiant flux is…

F - Radiant Flux
L - Luminosity
r - radius
So if a star is surrounded by a spherical shell and assuming that no light is absorbed when it exits the shell, the radiant flux can be measure in relation of the radius of the shell and the luminosity by the shown equation. A Greek astronomer named Hipparchus is actually one of the first one to notice this and he catalogs the stars. (My girlfriend is giving me the look like she wants me to “shut up.”) He assigns something called the apparent magnitude where m = 1 is the brightest and the scale goes up from there, so the higher the apparent magnitude, the dimmer it gets. Photometers can be used to measure these apparent magnitudes.  

I then proceeds to calculate the radiant flux, but not before finding the luminosity and radius values on my iphone. I also looked up the calculated valued  of the sun and show my girlfriend the two radiant flux and explains to her that Alpha Centauri appears less brighter because it is farther away whereas our sun is closer. (She stands up as I also rose, and she proceeds to smack me and say “We are through you Physics Nerd.” It was a really awkward trip back to California when she tries to make me jealous by flirting with another guy on the plane. Never saw her again.) TRUE STORY OR IS IT? :D 

Thursday, January 12, 2012

Make A Wish


Parseid Meteoroids (13 August 2011)
Have you ever make a wish on a shooting star? I know I have. When we were young, we are told by parents and friends that wishing upon a shooting star might make our wish come true. But do you know what a shooting star really is? Shooting stars travel so incredibly fast that it is almost impossible to take a picture on Earth, so here is a shooting star from an angle in space.The meteoroids got pull in by the Earth's gravitation and the shooting star that we see is just the meteoroids actually breaking up upon entering Earth's atmosphere. The glowing taillight of the shooting star is called a vapor trail or streak, this means that the meteoroids is burning up when expose to air.


Did you notice that luminous yellow-green glow? Do you know what it is?


This one of many things an astronomer would do, because their job is to classify and describe the things in space. This might include planets, stars, galaxies, meteors, etc. You do not need a degree in Astronomy to be an astronomer! Having a telescope and looking up in space as you observe the various changes of the planets and stars already makes you an astronomer. So the next time you see a shooting star, don't close your eyes to make a wish, but rather look closely at its vast beauty burning up because they do travel very fast. (About 26 miles per second)