Skip to content
Starts With A Bang

Ten Solstice Facts That Everyone Should Know

It’s where Earth’s axial tilt with respect to the Sun is most extreme. Here are the consequences.

Today is June 21st, 2019: the day of the solstice. Although there are many factors at play that determine the behavior of each planet — its spin and orbital angular momenta, the eccentricity of its orbit, the effects of General Relativity and the other planets — there’s only one that determines when the solstices are: axial tilt. As every planet revolves around the Sun, it rotates on its axis, and only the orientation of that axis matters.

Even though the Earth always rotates on its axis, which is tilted at 23.5 degrees, the equinoxes are special for having that axial tilt be perpendicular to the Sun-Earth plane, rather than at an angle, which occurs on all other days of the year. Similarly, the solstices are what occurs at the midpoints between the equinoxes: when the Earth’s axis is maximally tilted with respect to the Earth’s orbital plane around the Sun. (LARRY MCNISH / RASC CALGARY CENTRE)

Dependent on which side of the equator you’re on, you’ll experience the summer solstice when your hemisphere (north or south) is maximally tipped towards the Sun, and the winter solstice when your hemisphere is maximally tipped away from the Sun. The solstices are colloquially known as the longest or shortest day of the year. While this is true, they represent so much more than that. Here are the facts that everyone should know.

The observed path that the Sun takes through the sky can be tracked, from solstice to solstice, using a pinhole camera. That lowest path is the winter solstice, where the Sun reverses course from dropping lower to rising higher with respect to the horizon, while the highest path corresponds to the summer solstice. (REGINA VALKENBORGH / REGINAVALKENBORGH.COM)

1.) Solstice literally means “Sun stands still” in Latin. If you were to trace out the path of the Sun in the sky throughout the year, such as with a pinhole camera (as shown above), you’d find that the Sun follows a set of paths that all correspond to it rising somewhere in the east/northeast/southeast, reaching a maximum height overhead, and setting somewhere in the west/northwest/southwest.

But over the course of a year, one path will be the longest and reach the highest point, while another path will be the shortest and reach the lowest maximum height above the horizon. These correspond to the solstices: winter and summer solstice, to be precise. The reason it’s called the solstice is because — for approximately a week on either side of the solstices — the apparent change in motion of the Sun is largely imperceptible. The Sun appears to “stand still,” and the word solstice comes from the Latin “sol” (for Sun) and the verb “stare” (to be fixed/rigid/unmoving).

As the Earth rotates on its axis and orbits the Sun in an ellipse, the Sun’s apparent position appears to change from day-to-day in this particular shape: Earth’s analemma. The tilt of the analemma will correspond to the time of day at which the image is taken, but this shape is always reproduced from Earth if you take a photograph at the same time of every day. (GIUSEPPE DONATIELLO / FLICKR)

2.) The tips of any analemma you can construct occur on the solstices. If you were to photograph the Sun at the same exact time, every day, for 365 days, you’d find that it traces out a particular shape known as the analemma, which looks like a figure 8 on our world. Defined by both our planet rotating on its tipped axis and our elliptical motion around the Sun, the analemma will rotate throughout the day.

But the uppermost tip of the analemma, if you were to draw an imaginary line down the long axis of it, always occurs at the summer solstice, while the lowest tip occurs at the winter solstice. This is highly related to the pinhole camera picture you saw earlier, but it’s a fun fact that this remains true regardless of the time at which you look at the Sun. So long as you’re consistent from day to day throughout the year, the analemma’s extreme tips will indicate the solstices.

With a large amount of atmosphere to pass through, light from the Sun (or Moon) reddens tremendously when it’s close to the horizon. Neither the latest sunset of the year nor the earliest sunrise of the year corresponds to the summer solstice. (MAX PIXEL / FREEGREATPICTURE.COM)

3.) The solstices, despite being the longest and shortest days of the year, do not correspond to the earliest or latest sunrises and sunsets. Since the winter solstice corresponds to the shortest day of the year, with the least amount of sunlight, then you might expect you’d see the latest sunrise and the earliest sunset of the year on that day. Similarly, since the summer solstice is the longest day of the year, you’d be reasonable to expect the earliest sunrise and the latest sunset of the year.

But this isn’t the case for any of these expectations. While the Earth’s axial tilt determines solstice and equinox, the ellipticity of our orbit helps determine the time of earliest sunrise and latest sunset. The naive expectation would only be true if our orbit was a perfect circle. As it stands, the earliest sunrise occurs before the June solstice and the latest sunset occurs after the June solstice. The farther away from the equator you are, the closer these dates will be to the solstice, while the closer to the tropics, it might be as far as two weeks away.

Just 800 years ago, perihelion and the winter solstice aligned. Due to the precession of Earth’s orbit, they are slowly drifting apart, completing a full cycle every 21,000 years. 5,000 years from now, the spring equinox and the Earth’s closest approach to the Sun will coincide. (GREG BENSON AT WIKIMEDIA COMMONS)

4.) The solstices are unrelated to the planet’s closest approach to or farthest distance from the Sun. You might notice that the December solstice is very close in time to Earth’s perihelion, where it makes its closest approach to the Sun, occurring in early January. Similarly, the June solstice is very close in time to Earth’s aphelion, or its farthest distance from the Sun, occurring on July 4th of this year.

But this is only a coincidence. Earth’s orbit is an ellipse, and this ellipse precesses over time. With a period of about 21,000 years, the winter solstice will line up with perihelion and then move farther away, lining up with aphelion 10,500 years later, and then another 10,500 years on, with perihelion once again. The alignment was perfect 800 years ago, and we won’t have another solstice/perihelion/aphelion alignment for approximately 10,000 years to come.

During the winter solstice, the closer to the pole you are, the lower the Sun appears at every moment, including at its highest, above the horizon. From Fairbanks, AK, as shown here on the winter solstice, it never gets more than a few degrees above the horizon. For everyone at a latitude greater than 43 degrees, on your winter solstice, the Sun never reaches higher above the horizon than an observer at the opposite pole will see it all day long. (KEN TAPE)

5.) If you live at a higher latitude than the 43rd parallel, the Sun is lower during your winter solstice than it is at the opposite hemisphere’s pole. Are you a fan of Santa Claus, and his apocryphal home at the North Pole? As Santa experiences the summer solstice, the Sun will continuously appear, today, at a height of 23.5° above the horizon. This is higher than the highest angular height above the horizon of any observer south of 43° latitude in the southern hemisphere.

This includes cities like: Christchurch and Dunedin in New Zealand; Port Arthur, Bruny Island and Cape Raoul in Tasmania; Comodoro Rivadavia, the Falkland Islands, and Santa Cruz province in Argentina; about the southernmost third of Chile, and the entire continent of Antarctica.

The Sun’s apparent path through the sky on the solstice is vastly different near the equator, at 20 degrees latitude (left) versus far from the equator, at 70 degrees latitude (right). If you’re at greater than a 66.5° latitude, you will have either 0 or 24 hours of sunlight during the solstice, depending on whether it’s the winter or summer solstice. (WIKIMEDIA COMMONS USER TAUʻOLUNGA)

6.) Observers within the Arctic/Antarctic circle on the solstice will either see 0 or 24 hours of sunlight. Because our Earth is tilted on its axis at 23.5°, anyone living at a latitude higher than 66.5° (because 90° — 23.5° = 66.5°) will either never have the Sun rise above the horizon (during the winter solstice) or set below the horizon (during the summer solstice).

This is at its least extreme at the border of the Arctic/Antarctic circles themselves, were the Sun almost appears to rise/set and then dips a full 23.5° above or below the horizon 12 hours later. But at the north or south poles, you’ll receive 6 consecutive months of night followed by 6 consecutive months of sunlight. Things switch only on the equinoxes: the mid-way point between the two solstices.

No one has ever taken a 360-degree star trail photo from Earth before. This photo was actually a 12-hour exposure, on a mount scheduled to rotate at a rate of 15-degrees-per-hour to create the almost 360-degree effect. (EARL MOSER, VIA ASTRO-TOM.COM)

7.) The solstices mark the most favorable time for taking the first-ever 360° star trail photo. The Earth rotates on its axis once every 24 hours, and the Sun has to be about 12° to 18° below the horizon in order for the sky to darken enough to reveal a substantial number of stars. If you’re close enough to the appropriate pole (north or south) during the winter solstice, and your skies are clear, you just might get a continuous 24 hour view of the stars.

This would enable a lucky observer to complete what’s known as Lewin’s Challenge, which is the endeavor to photograph (with no tricks) a set of complete, 360° star trails. Technically, an observer at the South Pole has about 5 weeks on either side of the solstice to try and accomplish this. Clear skies at the poles during winter are rare, but if you’re already at the poles, you owe it to yourself to try!

When the Earth’s north pole is maximally tilted away from the Sun, it’s maximally tilted towards the full Moon, on the opposite side of the Earth, while when your hemisphere of the Earth is maximally tilted towards the Sun, it’s maximally tilted away from the full Moon. The Moon stabilizes our orbit but also slows the Earth’s rotation. The total inclination of the Moon’s orbit, of 5.1°, represents the maximum possible variance from a perfect Moon-Earth-Sun alignment.(NATIONAL ASTRONOMICAL OBSERVATORY ROZHEN)

8.) The full Moon closest to the solstice will trace the maximally opposite path of the Sun. When the Earth’s axis is maximally tilted towards the Sun and the Moon is full — as in, on the other side of the Earth from the Sun — that means the Earth’s axis will be maximally tilted away from the Moon. To within a variance of just 5 degrees, Earth-Moon orbital plane’s inclination, the time when the Sun appears to carve its highest path through the sky, the full Moon is carving its lowest path through the sky.

The exact opposite is true during the winter solstice: the Earth’s axis is maximally tilted towards the full Moon and away from the Sun. If you caught Monday’s full Moon, it marked the highest full Moon of the year for observers south of the equator, while it marked the lowest full Moon of the year for northern hemisphere observers. If you come back for the full Moon of December 12, 2019, you’ll catch the same phenomenon, except for opposite hemispheres.

Two-hemisphere global composites of Moderate Resolution Imaging Spectroradiometer (MODIS) data, taken in 2001 and 2002. Note that it’s our oceans, and our oceans alone, that give our planet its blue appearance from space, and also cause a tremendous offset between the solstices and the temperature extremes we experience. (NASA / BLUE MARBLE PROJECT)

9.) The solstices are neither the hottest nor coldest days of the year. This one is actually very specific to Earth: the hottest times of the year typically correspond to approximately 6 weeks after the summer solstice, and the coldest are approximately 6 weeks after the winter solstice. Other planets don’t have this same phenomenon for one very important reason: they don’t have the majority of their surfaces covered in liquid water.

The oceans themselves, being composed of large quantities of water and containing approximately 1,000 times the mass of Earth’s atmospheres, contain a tremendous amount of heat, and are slow to change their temperatures. We might receive more (or less) energy from the Sun on the summer (or winter) solstices, but the oceans require time to heat up or cool down. Global average temperature extremes, therefore, usually occur in early August and February, rather than at the June and December solstices.

On June 21, 2004, SpaceShipOne was launched, becoming the first privately-funded human spaceflight, and marking the unofficial dawn of the era of commercial astronauts. (D RAMEY LOGAN / WIKIMEDIA COMMONS / CCA-SA-3.0)

10.) The June and December solstices mark two incredible milestones in space exploration. In 2004, SpaceShipOne completed its maiden suborbital space flight on the summer solstice: June 21. Today, therefore, is the 15th anniversary of the unofficial start of the era of commercial spaceflight. It’s a stark contrast to the space exploration milestone that occurred much longer ago on the other solstice.

Travel the Universe with astrophysicist Ethan Siegel. Subscribers will get the newsletter every Saturday. All aboard!

On the December solstice, the Apollo 8 mission, the first crewed mission to reach and orbit the Moon, was launched in 1968. Frank Borman, Jim Lovell and Bill Anders became the first humans to view Earth from such a great distance, beginning their journey away from our planet on the darkest evening of the year. Three days later, they plunged behind the Moon, rendering both the Sun and the Earth invisible for a few hours. When the Sun and then the Earth re-emerged over the limb of the Moon, they saw this breathtaking sight.

The first view with human eyes of the Earth rising over the limb of the Moon. The discovery of the Earth from space, with human eyes, remains one of the most iconic achievements in our species’ history. Apollo 8, which occurred during December of 1968, was one of the essential precursor missions to a successful Moon landing, which will celebrate its 50th anniversary this July. Note the blue color of Earth is due to the oceans, not the atmosphere. (NASA / APOLLO 8)

As Bill Anders said almost immediately,

We came all this way to explore the Moon, and the most important thing is that we discovered the Earth.

Enjoy the solstice however you see fit, and as you do, try and remember this: whether you’re bathed in the longest day or the longest night of the year, there are some things that we all have in common and can bring us all together. The story of where we are and how we came to be here — on Earth, in the Solar System and in the Universe — just might be the most omnipresent of them all.

Ethan Siegel is the author of Beyond the Galaxy and Treknology. You can pre-order his third book, currently in development: the Encyclopaedia Cosmologica.


Up Next