Astronomy EssentialsSpace

3200 Phaethon is the Geminid meteors’ mysterious source

3200 Phaethon: An asteroid-like body (round rock), venting gases into space.
Artist’s concept of asteroid 3200 Phaethon. The sun may heat the asteroid’s surface enough that sodium inside it would vaporize and vent into space, making it brighten like a comet. It might also dislodge small pieces of rocky debris. Image via NASA/ JPL-Caltech/ IPAC.

2022’s Geminid meteor shower is expected to peak on the morning of December 14. This year, a bright waning gibbous moon will be above the horizon during the peak time (around 2 a.m.) for viewing the meteors. Luckily, the radiant point rises in mid-evening. So there will be a window of darkness – on both the evenings of December 13 and 14 – from mid-evening until moonrise around midnight. Read more about 2022’s Geminid meteor shower.

Weirdly comet-like 3200 Phaethon

Most meteors in annual showers have comets as their sources. But not December’s Geminid meteors, whose source, known as 3200 Phaethon, is a strange hybrid of an asteroid and a comet. This “rock-comet” isn’t icy, like a comet is. But it’s known to brighten as it nears the sun, as comets do. And it has a tail. Plus, it spawns the Geminid meteor shower. And so scientists puzzle over 3200 Phaethon. How can a rocky asteroid leave behind debris that sparks a meteor shower? Where does its tail come from?

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New research on 3200 Phaethon

On August 16, 2021, scientists with NASA’s Jet Propulsion Laboratory in Pasadena, California, announced a new idea that might help explain 3200 Phaethon’s comet-like behavior. Part of the answer might be sodium fizzing from the asteroid’s surface. Their statement explained that this asteroid:

… brightens as it gets close to the sun. Comets typically behave like this: When they heat up, their icy surfaces vaporize, causing them to become more active and brighten as the venting gases and dust scatter more sunlight. But what is causing Phaethon to brighten if not vaporizing ices?

The culprit could be sodium. As the new study’s authors explain, Phaethon’s elongated, 524-day orbit takes the object well within the orbit of Mercury, during which time the sun heats the asteroid’s surface up to about 1,390 F (750 C). With such a warm orbit, any water, carbon dioxide or carbon monoxide ice near the asteroid’s surface would have baked off long ago. But, at that temperature, sodium may be fizzing from the asteroid’s rock and into space.

Sodium in the mix

Astronomer Joe Masiero of IPAC at Caltech is lead author of the new study. He said:

We know it’s an asteroid and the source of the Geminids. But it contains little to no ice, so we were intrigued by the possibility that sodium, which is relatively plentiful in asteroids, could be the element driving this activity.

Gray background with line of dots and grid. A faint, fuzzy line connects some of the dots.
View larger. | Look closely to see the faint dust trail between the white dots. Asteroid 3200 Phaethon, parent body for the Geminid meteor shower, left this trail. The WISPR camera aboard the Parker Solar Probe captured this trail for the first time in 2019. At that time, astronomers said that something “catastrophic” might have happened to Phaethon a couple thousand years ago to create this trail of debris and the Geminid meteor shower. Now astronomers are wondering if sodium fizz is a better answer. Image via Brendan Gallagher/ Guillermo Stenborg/ U.S. Naval Research Lab.

Inspired by the Geminid meteors

Masiero and his team said observations of Geminid meteors inspired them. Their statement explained:

When meteoroids – small pieces of rocky debris from space – streak through Earth’s atmosphere as meteors, they disintegrate. But before they do, friction with the atmosphere causes the air surrounding the meteoroids to reach thousands of degrees, generating light. The color of this light represents the elements they contain. Sodium, for example, creates an orange tinge. The Geminids are known to be low in sodium.

Until now, it was assumed that these small pieces of rock somehow lost their sodium after leaving the asteroid. This new study suggests that the sodium may actually play a key role in ejecting the Geminid meteoroids from Phaethon’s surface.

[We] think that as the asteroid approaches the sun, its sodium heats up and vaporizes. This process would have depleted the surface of sodium long ago, but sodium within the asteroid still heats up, vaporizes, and fizzes into space through cracks and fissures in Phaethon’s outermost crust. These jets would provide enough oomph to eject the rocky debris off its surface.

So the fizzing sodium could explain not only the asteroid’s cometlike brightening, but also how the Geminid meteoroids would be ejected from the asteroid and why they contain little sodium.

Sodium dislodges particles

Björn Davidsson of NASA’s Jet Propulsion Laboratory is a co-author of the study. He added:

Asteroids like Phaethon have very weak gravity, so it doesn’t take a lot of force to kick debris from the surface or dislodge rock from a fracture. Our models suggest that very small quantities of sodium are all that’s needed to do this. It’s nothing explosive, like the erupting vapor from an icy comet’s surface. It’s more of a steady fizz.

Read more: Fizzing Sodium Could Explain Asteroid Phaethon’s Cometlike Activity

All that, and blue, too

By the way, the comet-like behavior of this asteroid isn’t the only unusual thing about it. For one thing, 3200 Phaethon has an odd color for an asteroid. Most asteroids are dull grey to red, depending on the type of material on their surface. 3200 Phaethon is blue. Blue asteroids are known, but make up only a fraction of all known asteroids. And Phaethon isn’t just blue. It’s one of the bluest of similarly colored asteroids (or comets) in the solar system.

Here’s another odd feature of 3200 Phaethon. While comets tend to have more elliptical orbits, asteroid orbits are more circular. 3200 Phaethon’s orbit – which is now exceedingly well known – is highly elongated, reminiscent of some comets. Its orbit crosses the orbits of Mars, Earth, Venus and Mercury.

Plus, its orbit brings 3200 Phaethon closer to the sun than any other named asteroid (though some smaller, unnamed asteroids come even closer). At its closest point, Phaethon is only 13 million miles (20.9 million km) from the sun. That’s less than half of Mercury’s closest distance.

The name of this object – 3200 Phaethon – honors its relationship to the sun, by the way. In Greek mythology, Phaethon was the son of the sun god Helios.

A potentially hazardous asteroid

3200 Phaethon is classified as a potentially hazardous asteroid. But that doesn’t mean it’s a threat to Earth. It just means two things. First, 3200 Phaethon is big. The latest estimates (2021) suggest it’s 3.6 miles (5.8 km) wide. It’s big enough to cause significant regional damage if it were to strike Earth. Second, it’s known to make periodic close approaches to Earth. But astronomers know of no upcoming strike by this object in the foreseeable future.

In 2017, 3200 Phaethon came closer to Earth than it will again until 2093. At its closest in 2017, it was still about 26 times the moon’s distance away.

Videos of 3200 Phaethon

Both amateur and professional astronomers watched 3200 Phaethon as carefully as they could in 2017. For example, Northolt Branch Observatories in London, England, created the animation below from images it captured in 2017.

Steven Bellavia also produced a video (below) of 3200 Phaethon in 2017. He commented then that he’d endured cloudy weather and subfreezing temperatures in order to capture the images.

Light gray oval rotating against dark gray background.
Astronomers at the Arecibo Observatory generated these radar images of 3200 Phaethon on December 17, 2017. Image via Arecibo Observatory/ NASA/ NSF/ Wikimedia Commons.

The history of 3200 Phaethon

3200 Phaethon was the first asteroid discovered via spacecraft, on October 11, 1983. Astronomers Simon F. Green and John K. Davies noticed it while searching Infrared Astronomical Satellite data for moving objects. Charles T. Kowal confirmed it optically and said it was asteroid-like in appearance. The object received the provisional designation 1983 TB. Two years later, in 1985, using the convention for naming asteroids, astronomers assigned it its asteroid number and name: 3200 Phaethon.

Before 3200 Phaethon, scientists linked all known meteor showers to comets and not asteroids.

Thus, 3200 Phaethon surprised them from the beginning, because – while it looked like an asteroid – it appeared to be the source of the annual Geminid meteor shower. Astronomers began calling 3200 Phaethon a comet-asteroid hybrid, an asteroid that behaves like a comet. Later, they began using the term rock-comet.

What else will we learn about this object, as the years pass?

Bottom line: The Geminid meteor shower has a unique source – 3200 Phaethon – sometimes called a comet-asteroid hybrid, or a rock-comet. In 2021, scientists suggested that some of this object’s comet-like behavior might stem from sodium fizzing from its surface.


Via U.S. Naval Research Lab

December 13, 2022
Astronomy Essentials

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