StarDate

The night sky can sometimes look like a tie-dyed T-shirt flapping on a clothesline. Ribbons and swirls of bright color ripple through the sky. They can change appearance in seconds – blown by the solar wind.

The colorful display is an aurora – the northern and southern lights. An aurora flares to life as charged particles from the Sun run into Earth at high speed.

Earth’s magnetic field funnels the particles toward the magnetic poles. When particles hit atoms and molecules high above the surface, they knock atoms out of their usual configuration. When they return to normal, the atoms emit light.

The color of an aurora depends on what the charged particles hit, and where they hit it. Most auroras are green. They switch on when particles hit oxygen molecules at altitudes of about 60 to 200 miles. Red auroras are fed by oxygen that’s even higher.

The lower fringes of a display can appear pink or dark red – the result of collisions with nitrogen at lower altitudes. Collisions with hydrogen and oxygen create blue and purple auroras. But they’re not very common, and they’re hard for the eye to take in. They’re easier to see in photographs.

Most of the time, the northern lights stay close to the magnetic pole. When the Sun spews out more particles, though, they can spread outward, shining in regions where they’re seldom seen. And the colors can get more intense – dramatically “tie-dying” the night sky.

Script by Damond Benningfield

The goddess of the dawn has given millions of Americans a rare treat the past couple of years: brilliant displays of the northern lights in regions where they’re seldom seen. Today, we know that these colorful curtains of light are powered by storms on the Sun. Bigger storms expand the viewing area. But in centuries past, cultures around the globe created their own explanations.

In Scandinavia, for example, the northern lights might have represented Bifrost, the “rainbow bridge” that connected Earth to Asgard, the home of the gods. In some of the islands of Scotland, the lights represented a pair of chieftains fighting for the hand of a “merry dancer.”

In southern England, they were considered omens of misfortune. Some saw the lights as clashing swords; red lights were streamers of blood. During an intense outburst in March 1716, at the end of a civil war, people ran into the streets in their nightclothes, and some thought it was judgment day. One writer said that some “read in its glaring visage, the fate of nations and the fall of kingdoms.”

The name for the northern lights – the aurora borealis – was bestowed in 1619 by Italian astronomer Galileo Galilei. Aurora was the Roman goddess of the dawn. Boreas was the Greek god of storms and the north wind – one of the namesakes of the always beautiful, sometimes frightening northern lights.

More about the aurora tomorrow.

Script by Damond Benningfield

Sixty years ago today, NASA was making its first attempt to land on the Moon.
Surveyor 1 had been launched three days earlier.

The robotic lander touched down in a crater in the Ocean of Storms – a giant volcanic plain. It was a precursor to the Apollo missions, which would land astronauts on the Moon.

Surveyor wasn’t the first probe to land on the Moon – a Soviet mission beat it by a few months. But Surveyor was more sophisticated. It carried a television camera to beam back images of its surroundings.

Surveyor transmitted its first pictures just minutes after landing. And during its first lunar “day” – almost 14 Earth days – it snapped more than 10 thousand images. They showed a surface coated with small rocks, and pockmarked by small craters. The rim of the crater Surveyor landed in was visible in the distance.

Pictures of its landing pads revealed important details about the texture of the lunar surface, as this NASA documentary pointed out:

 ANNOUNCER: The lunar surface texture not thick layers of loose dust into which spacecraft or men could sink. In the area of the Ocean of Storms, man can land and walk on the lunar surface.

Surveyor 1 survived the frigid lunar night, taking hundreds more pictures the next day. Scientists even raised it the following January – seven months after its historic landing on the Moon.

Script by Damond Benningfield

The twins of Gemini have a front-row seat for a planetary waltz this month. Venus, Jupiter, and Mercury are close to the twins now, and will bunch up even closer as the month progresses.

The “twins” are the stars Pollux and Castor. They’re about a quarter of the way up the western sky as evening twilight fades. Pollux is the brighter of the two, with Castor to its right.

Jupiter looks like a brilliant star to the lower left of the twins. It’s the largest planet in the solar system. But it’s on the far side of the Sun as seen from Earth, so it’s more than 550 million miles away – about six times the distance between Earth and the Sun.

Venus is even brighter – the “evening star.” It’s below the twins. Although it’s a little smaller than Earth, it shines much brighter than Jupiter mainly because it’s much closer to both Earth and the Sun.

Venus and Jupiter remain in view for a good while after darkness falls. That’s not the case for Mercury. It’s well to the lower right of the others, and much lower in the sky. It’s bright, though, so with a clear horizon, there’s a good chance to spot it.

Mercury will move a little higher into the sky over the next few nights, improving the view. But the real action involves Jupiter and Venus. Venus is climbing away from the Sun quickly. It will nestle especially close to Jupiter on the 8th and 9th. It’ll pull away after that – all in close view of the twins.

Script by Damond Benningfield

It’s early in the long winter night at the south pole. But a few dozen scientists and others have settled in at a research base there. They monitor the weather and climate, listen to rumbles in the ice below, and watch auroras dancing in the dark skies above. And they operate observatories that study the universe beyond.

One of those observatories is buried in the ice. Known as IceCube, it’s a set of thousands of light detectors. They look for evidence of neutrinos – particles that are produced in the Sun, exploding stars, and other powerful objects and events. They almost never interact with other matter. But when one does interact, by smashing into an ice molecule, it produces a quick flash of light. Studying that flicker reveals details about the neutrino, including its origin. And that tells scientists more about the body that created it.

Another observatory, the South Pole Telescope, studies the “afterglow” of the Big Bang. Known as the cosmic microwave background, it’s a sort of “haze” that fills the entire universe. Tiny fluctuations in the haze reveal details about the birth of the first stars and galaxies.

Water vapor in the atmosphere absorbs microwaves. But the south pole is almost two miles high, and it’s so cold that there’s almost no water vapor in the skies above it. That allows the 10-meter dish to study the background glow in great detail – under the clear, dark skies at the bottom of the world.

Script by Damond Benningfield