Stanford SOLAR Center -- Ask A Solar Physicist FAQs (2024)

Why does the Sun appear orange?Stanford SOLAR Center -- Ask A Solar Physicist FAQs (1)

(by Amara Graps)

The subject of the perception of colors has many facets- thepsychological aspects, the physiological aspects, the physicalaspects, among others.

Color is an interesting and complex subject. If you would like tounderstand colors in a complete way, I suggest starting with PaulHewitt's _Conceptual Physics_ Chapter 27: "Color", and then browsingthrough: M. Minnaert's _The Nature of Light and Color in the OpenAir_ (A Dover Press book).

Also, in your question, you are talking as if the Sun is appearingorange in color. I'm assuming that you are seeing it with your nakedeye, such as a setting Sun, low on the horizon, rather than seeing theSun through an orange filter. (Note that it is dangerous to lookdirectly at the bright Sun!)

What I say below is from Paul Hewitt's _Conceptual Physics_.

Strictly speaking, the colors that you see are not in the emittingsubstances, or even in the light that they reflect because color is a*physiological* experience and therefore dependent on the individualviewing the object. Color is in your head. So an apple *appears* red,the setting Sun *appears* orangish-red, and so on.

The physics of colors is the following. The colors that we seedepends on the frequency of the emitted light. Different frequenciesof light are perceived as different colors: the lowest frequency beingred, the highest violet, and in-between those two are the infinitenumber of hues that make up the color spectrum of the rainbow. Thefrequency of the emitted light depends on electron transitions betweenthe atomic energy levels of the source. However, most objects_reflect_ rather than _emit_ light, and they reflect only part of thelight that is shining on them- the part that gives them their color.

Your question points out differences in color one sees due to emitted and reflected and transmitted light.

An apple appears red because in white light, the apple _reflects_ thered part of the white light. (Try looking at an apple using aprism. If you pass sunlight through a prism in order to generate aspectrum, and hold the apple in each of the dominating colors, youwill notice the color of the apple changing.))

We see the Sun however, mostly as an _emitting_ and _transmitting_object through our Earth atmosphere. These two factors make ourperception of the Sun's colors as a different phenomena than lightreflection of an object such as a red apple.

The Sun *emits* white light, which is actually a composite of all ofthe visible frequencies of light. (A prism shows you the visiblefrequencies of white light.) The distribution of solar frequencies isuneven, the most intense frequency is in the yellow-green part of thespectrum. All of the visible frequencies mixed together producewhite. (Note that this white also results from the combination of onlyred, green, and blue light (the additive primary colors).)

Our Earth atmosphere predominately contains nitrogen and oxygenmolecules. These atoms behave as behave like tiny optical tuning forksand selectively scatter light waves of appropriate frequencies. Thenatural frequencies that nitrogen and oxygen resonate with thesunlight at are in the ultraviolet part of the white light solarspectrum. Visible violet light has a frequency close to theultraviolet frequencies, so there is considerable forced vibrations,and therefore, violet light scatters in our atmosphere in largeamounts. For every ten violet photons scattered from a sunlight beam,only one red photon in scattered. Some blue light, and a little bit ofgreen light, scatter in similar ways, so that is why the sky appearsblue.

Red, orange and yellow light are lower frequencies of light than blueand green. These lower frequencies are scattered the least by nitrogenand oxygen. Therefore, red, orange, and yellow light are transmittedthrough our atmosphere more readily than blue. (Red, which isscattered the least amount, traverses more atmosphere relativelyunhindered than any other color.) Do you see now that we are notseeing the effects of reflection, like from an apple? We are seeingthe consequences of emitted and transmitted light.

Therefore when we see the Sun setting, a white-light-emitting object,through our thick Earth atmosphere, the higher frequencies arescattered while the lower freqencies are transmitted. At sunset, whenthe Sun is lowest in the sky, and seen through the largest amount of"air mass", we see it as an orangish-red color.

You may also enjoy this article on The Color of the Sun

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Stanford SOLAR Center -- Ask A Solar Physicist FAQs (2024)

FAQs

Why does it have to be so hot at the center of the sun to fuse hydrogen to helium? ›

A high temperature helps because it makes the hydrogen nuclei move faster. They need this extra speed so that they can get close together and join.

How does the sun create energy? ›

Solar energy is created by nuclear fusion that takes place in the sun. Fusion occurs when protons of hydrogen atoms violently collide in the sun's core and fuse to create a helium atom. This process, known as a PP (proton-proton) chain reaction, emits an enormous amount of energy.

What temperature is required for hydrogen fusion? ›

The minimum temperature required to fuse hydrogen is about 100 million Kelvin, which is about six times the temperature in the core of our Sun. The pressure required must be high enough to force the hydrogen nuclei within 10^(-12) millimeters of each other.

What pressure is needed for fusion? ›

Fusion energy requires confinement of a very hot plasma at a high pressure. The magnetic confinement approach uses strong magnetic fields to confine a very hot—many times hotter than the center of the sun—plasma with pressures up to 10 times the atmospheric pressure at Earth's surface.

What is the biggest challenge of using solar energy to generate electricity? ›

One of the biggest problems that solar energy technology poses is that energy is only generated while the sun is shining. That means nighttime and overcast days can interrupt the supply.

What places on Earth might have the best capacity for solar power? ›

These factors are latitude, cloud cover, aerosols, elevation and shading. Not surprisingly, the site with the highest solar energy potential on Earth happens to be near the equator, surrounded by an arid climate away from major sources of pollution, and it also happens to be on a plateau.

What will happen to Earth without the Sun's energy? ›

Without the Sun , Earth's land, water, and air would all be frozen solid! Life on Earth would cease to exist. That's because almost all living things rely on the steady light and heat of the Sun. The Sun's heat makes liquid water on our planet possible.

How did the Sun get hot enough to begin fusing hydrogen into helium? ›

The Sun was born about 4.6 billion years ago from the gravitational collapse of a vast cloud of gas and dust. Material in the center of the cloud was squeezed so tightly that it became hot enough to ignite nuclear fusion. Today, the Sun continues to fuse hydrogen atoms to make helium in its core.

Why does fusion need to be hotter than the Sun? ›

Temperature. Plasmas need to be hot. While fusion occurs in the sun's core at a temperature of 15 million degrees Celsius, fusion on Earth must exceed this temperature by several orders of magnitude to account for lower atmospheric pressure.

How does the Sun turn hydrogen into helium? ›

Fusion reactions occur when two nuclei come together to form one atom. The reaction that happens in the sun fuses two Hydrogen atoms together to produce Helium. It looks like this in a very simplified way: H + H → He + ENERGY.

What will happen when the Sun begins to fuse helium in its core? ›

When the temperature in the core reaches about 100 million degrees, the helium will begin to fuse into carbon by a reaction known as the triple-alpha process, because it converts three helium nuclei into one carbon atom. This generates a great deal of heat.

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