The Sun

The Sun today from your location

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This panel computes today's sunrise, sunset and day length for the Sun in your browser, and it needs JavaScript to run. The rest of this page, including the calendars and event dates below, is fully readable without it. For a live all-sky view, open the Sky Map or Today in the Sky.

Everything is computed on your device. Tapping "Use my location" sends your coordinates once to a place-name service only to show your city's name. Times appear in your device's time zone.

The Sun at a glance

Physical data: NASA NSSDCA Sun Fact Sheet and NASA Science.

Equinoxes, solstices and Earth's orbit

The seasons turn on four instants a year: two equinoxes, when the Sun crosses Earth's equator, and two solstices, when it reaches its farthest point north or south. Separately, Earth's slightly elliptical orbit brings us closest to the Sun in early January and farthest in early July, a rhythm that does not cause the seasons but does fine-tune their lengths. Dates are in Universal Time.

How to see the Sun

Safety comes before everything else with this target: never look directly at the Sun. It can injure the retina in moments, and because the retina has no pain receptors, the damage arrives without warning. There are only three safe ways to observe it: certified eclipse glasses meeting the ISO 12312-2 standard, a purpose-made solar filter fitted over the front of a telescope or binoculars, or projection, described below. Never look through any optics pointed at the Sun unless a certified filter covers the front; ordinary sunglasses, smoked glass, and filters that screw into the eyepiece are all unsafe.

Projection is the free method. Make a small, clean hole in a piece of card, stand with your back to the Sun, and let sunlight pass through the hole onto a second card a few feet away: the bright circle it forms is a true image of the Sun's disk. A kitchen colander throws dozens of these images at once, and during a partial eclipse every one of them becomes a tiny crescent.

Telescope projection is also how to watch sunspots, and it is the one arrangement where a telescope is aimed at the Sun without a filter: the image falls on a card, and no eye ever goes anywhere near the eyepiece. Cap or remove the finder scope first, point a small telescope at the Sun by minimizing its shadow (never sight along the tube), and project the eyepiece image onto white card; a simple refractor works best for projection, and never leave the setup unattended where a child could put an eye to it. The other route is a proper white-light filter over the front aperture, which makes looking through the eyepiece safe. Either way you can follow dark spots drifting across the disk as the Sun rotates, multiplying and fading with the roughly 11-year solar cycle. A small telescope used this way shows a pale, quiet disk carrying a few dark spots, far short of the seething detail in the spacecraft image on this page. Prominences and flares need specialized hydrogen-alpha telescopes, which isolate a single deep-red wavelength of hydrogen light.

The Sun's cycles

Watched from Earth, the Sun sets the rhythm of the day and the year. Because Earth's axis is tilted, the Sun rides high in summer and low in winter, and its rising and setting points sweep along the horizon through the year; the seasons lesson shows why the tilt, not distance, does the work (Earth is actually closest to the Sun, about 147 million kilometers, during northern winter). The Sunrise and Sunset Calculator charts the whole yearly swing for your location, and the equation of time lesson explains the subtler rhythm that makes sundial noon and clock noon drift apart and back over the year.

The Sun also keeps a cycle of its own. It does not rotate as a solid body: the equator turns in about 25 days while regions near the poles take up to 36. That uneven spin winds up the solar magnetic field, which erupts through the surface as sunspots, and their numbers rise and fall over a cycle averaging roughly 11 years. The sunspot cycle lesson lets you explore centuries of real sunspot counts and see the rhythm for yourself.

Eclipses depend on a coincidence of scale. The Sun's disk spans about half a degree of sky, so close to the Moon's apparent size that the Moon can only just cover it. The Eclipse Explorer maps every upcoming solar eclipse and shows where each one is visible.

The slowest rhythms dwarf human history. Over tens of thousands of years, gradual shifts in Earth's orbit and tilt redistribute sunlight and pace the ice ages, the Milankovitch cycles. And the Sun is itself a traveler, carrying the whole solar system around the Milky Way at about 720,000 kilometers per hour: one galactic year takes roughly 230 million years.

To see where these periods fit among everything else that repeats overhead, find the sunspot cycle in the full list, sorted by length, on the Cycles page.

What's next for the Sun

The Sun's headline events are eclipses, the only times the solar disk itself puts on a show for the naked eye (through proper eclipse glasses, always). The Eclipse Explorer maps where each one is visible. Dates are in Universal Time.

Frequently asked questions

Why is it dangerous to look at the Sun during an eclipse?

Because even a thin sliver of the exposed Sun is intense enough to burn the retina, and the retina feels no pain, so the damage happens without warning. A partial eclipse is especially risky: the sky dims, your pupils open wider, and staring feels easier than usual. Certified eclipse glasses meeting ISO 12312-2, a purpose-made solar filter over the front of a telescope or binoculars, or projection are the only safe options. Naked-eye viewing is safe only during the brief total phase of a total eclipse, while the Moon completely covers the Sun's disk.

How long does sunlight take to reach Earth?

About 8 minutes. The Sun is on average 149.6 million kilometers away, and light crossing that gulf takes a little over eight minutes, so you always see the Sun as it was roughly eight minutes ago. The distance varies through the year, between about 147 and 152 million kilometers, which changes the travel time by about eight seconds either way.

Does the Sun orbit anything?

Yes. The Sun orbits the center of the Milky Way galaxy, carrying the planets along with it at about 720,000 kilometers per hour. One full lap, sometimes called a galactic year, takes about 230 million years. Since the Sun is roughly 4.5 billion years old, it has completed only about 20 of these laps in its entire lifetime.

What is the solar cycle?

The solar cycle is the rise and fall of the Sun's magnetic activity over a period averaging a little over 11 years. At solar maximum the disk carries many sunspots and the Sun produces more flares and eruptions, which is when auroras are most frequent on Earth; at solar minimum the disk can be nearly spotless for weeks. Individual cycles run somewhat shorter or longer than the average.

What is the Sun made of?

Mostly hydrogen and helium. In the photosphere, the Sun's visible surface layer, about 91 percent of its atoms are hydrogen and about 9 percent are helium, with only traces of heavier elements such as oxygen, carbon and iron. The Sun is not burning in the ordinary sense: its core, at about 15 million degrees Celsius, fuses hydrogen into helium, converting more than four million tons of matter into pure energy every second.

When is the next solar eclipse?

The next solar eclipse anywhere on Earth is a total eclipse on August 12, 2026 (Universal Time), followed by an annular eclipse on February 6, 2027. Each eclipse is only visible from a limited region; the Eclipse Explorer on this site maps every path.

When is the next equinox or solstice?

The next is the September equinox on September 23, 2026 (Universal Time). The full table on this page lists every equinox and solstice for the next two years, with Earth's perihelion and aphelion dates alongside.

Keep exploring

• Sunrise and Sunset Calculator: today's sun times, twilight and day length for your location, all year
• Sunspot Cycle lesson: explore centuries of real sunspot counts behind the 11-year rhythm
• Eclipse Explorer: every upcoming solar eclipse and where its shadow falls
• Seasons lesson: why Earth's tilt, not its distance, makes summer and winter
• Equation of Time lesson: why sundial noon and clock noon disagree through the year