Sun

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Sunlight

Planetary Transits

Sun Rise & Set Calculators

Moon - Sun Interaction

Current Position of the Sun

Space Weather

http://umbra.nascom.nasa.gov/images/latest.html

Solar images at SDAC

Click on any of the following thumbnail images for the most recent, full-resolution solar image of each type in the SDAC archive. The time and date of each image is below the image description. The color tables used to display AIA images here are the ones used to display similar bandpasses for SOHO EIT and STEREO EUVI images. The color tables preferred by the AIA Principal Investigator Team can be found in the images at the LMSAL Sun Today site.
About this Menu Mar 19 Solar Region Summary Mar 18 Solar Region Summary http://www.swpc.noaa.gov/ftpmenu/forecasts/SRS.html

SRS

How the Sun Works"

http://www.howstuffworks.com/sun.htm When’s the last time you gazed upward and marveled at the mysterious, life-giving force that is the sun? If you believe the whole staring-at-the-sun-makes-you-go-blind thing (which is actually true), you’re probably not doing a whole lot of sun-gazing. But it’s a real marvel: The sun warms our planet every day, provides the light by which we see and is necessary for life on Earth . It can also cause cell death and make us blind.

Solar System Exploration: Planets: Sun: Overview

The sun is a star, a hot ball of glowing gases at the heart of our solar system. Its influence extends far beyond the orbits of distant Neptune and Pluto. Without the sun's intense energy and heat, there would be no life on Earth. And though it is special to us, there are billions of stars like our sun scattered across the Milky Way galaxy. Featured Mission: Solar Dynamics Observatory http://solarsystem.nasa.gov/planets/profile.cfm?Object=Sun
This Extreme Ultraviolet Imaging Telescope (EIT) image of a huge, handle-shaped prominence was taken on Sept. 14,1999. Taken in the 304 angstrom wavelength, prominences are huge clouds of relatively cool dense plasma suspended in the Sun's hot, thin corona. At times, they can erupt, escaping the Sun's atmosphere. Emission in this spectral line shows the upper chromosphere at a temperature of about 60,000 degrees K. Every feature in the image traces magnetic field structure. http://solarsystem.nasa.gov/multimedia/display.cfm?IM_ID=2166

Solar System Exploration: Multimedia: Gallery: Handle on the Sun

http://en.wikipedia.org/wiki/Sun

Sun - Wikipedia, the free encyclopedia

The Sun is the star at the center of the Solar System . It is almost perfectly spherical and consists of hot plasma interwoven with magnetic fields . [ 10 ] [ 11 ] It has a diameter of about 1,392,000 km, about 109 times that of Earth , and its mass (about 2 × 10 30 kilograms, 330,000 times that of Earth) accounts for about 99.86% of the total mass of the Solar System. [ 12 ] Chemically, about three quarters of the Sun's mass consists of hydrogen , while the rest is mostly helium . The remainder (1.69%, which nonetheless equals 5,628 times the mass of Earth) consists of heavier elements, including oxygen , carbon , neon and iron , among others. [ 13 ]

Sun: Rise, set times, solar eclipse dates, sun facts

The Sun Is Really Far Away The Sun is about 93 million miles away from Earth. The actual distance varies during Earth's orbit, which is elliptical, or oval, not round. http://www.almanac.com/sun
Equinoxes, Solstices, Crossquarter Days