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2 Pallas

Adapted from Wikipedia · Adventurer experience

An image of the asteroid Pallas, showing its cratered surface and unique topological features as captured by the Very Large Telescope.

2 Pallas (minor-planet designation: 2 Pallas) is the third-largest asteroid in the Solar System. It was the second asteroid ever found, after Ceres. Scientists think it might be a piece left over from when planets were made.

Like Ceres, Pallas is made of materials found in some meteorites, but it has less water than Ceres. Pallas is very big—it’s about three-quarters the size of Vesta and makes up around 7% of all the material in the asteroid belt.

Long ago, many pieces like Pallas came together to form planets. Most became part of the planets we see today, but some didn’t. Pallas, along with Vesta and Ceres, is one of the few big pieces that survived.

Pallas was discovered in 1802 by a German astronomer named Heinrich Wilhelm Matthias Olbers. At first, it was thought to be a planet. But as more small worlds were found, scientists began to call them “asteroids.”

Pallas has a tilted path around the Sun. Because of this tilt, it can get very close to some stars. On October 9, 2022, it passed very near the bright star Sirius.

History

On the night of April 5, 1779, the astronomer Charles Messier saw an object that looked like a star while tracking a comet.

Later, in 1801, another astronomer named Giuseppe Piazzi found a moving object that wasn’t a comet. This was the first asteroid ever discovered and was named Ceres.

Soon after, another astronomer named Heinrich Olbers noticed yet another moving object nearby. This was the asteroid Pallas, the second asteroid to be discovered. Finding Pallas sparked excitement because some astronomers had guessed there might be a planet between Mars and Jupiter.

The orbit of Pallas was calculated by Carl Friedrich Gauss, showing it takes about 4.6 years to go around the Sun, similar to Ceres. Pallas also has a tilted path compared to most objects in space.

Orbit and rotation

Pallas moves in a special way around the Sun. Its path is tilted and not a perfect circle, even though it is far from the Sun like most objects in the asteroid belt. Pallas also tilts on its side by 84°. This means that some parts of it get constant sunlight or darkness for a long time — even up to two of our years near the poles.

Near resonances

Pallas has a high eccentricity and a highly inclined orbit

Pallas shares its orbit with another big object called Ceres, though this is likely by chance. Pallas has special patterns in its orbit with Jupiter, happening roughly every 91,000 years and every 83 years.

Animation of the Palladian orbit in the inner Solar System 
-     Pallas
-     Ceres
-     Jupiter
-     Mars
-     Earth
-     Sun

-

An animation of Pallas's near-18:7 resonance with [Jupiter](/wiki/Jupiter). The orbit of Pallas is green when above the ecliptic and red when below. It only moves clockwise: it never stops or goes backward (i.e. no [libration](/wiki/Libration)). The motion of Pallas is shown in a reference frame that rotates about the [Sun](/wiki/Sun) (the center dot) with a period equal to Jupiter's orbital period. Accordingly, Jupiter's orbit appears almost stationary as the pink ellipse at top left. [Mars](/wiki/Mars)'s motion is orange, and the Earth–Moon system is blue and white.

Transits of planets from Pallas

From Pallas, we can sometimes see planets like Mercury, Venus, Mars, and Earth passing in front of the Sun. Earth last did this in 1968 and 1998 and will do so again in 2224. Mercury did so in October 2009. Venus will next do this in 2123, and Mars will in 2759.

Physical characteristics

Relative sizes of the four largest asteroids. Pallas is second from right.

Pallas is the third-largest asteroid in our solar system. It is slightly smaller than 4 Vesta but still very big. Pallas is made of materials similar to some meteorites on Earth, but it has less water than 1 Ceres.

Pallas is covered in craters from impacts. It is not perfectly round, which suggests it may have been hit by a large object in the past. Its surface has one bright spot and many large craters.

Satellites

Scientists once thought they saw a small moon around 2 Pallas in 1978, but later they learned this was not true. In 1980, they thought they found a bigger moon, but more data showed that was not right either.

Exploration

The asteroid 2 Pallas has never been visited by a spacecraft, but there have been ideas to send one. One idea was for a spacecraft called Dawn, which visited 4 Vesta and 1 Ceres, to also fly by Pallas. This wasn't possible because Pallas orbits at a steep angle. Another idea was a mission called Athena SmallSat, which would have flown by Pallas in 2022. However, this mission wasn't chosen.

Images

Artist's impression of potential dwarf planets and celestial bodies in our solar system.
A colorful montage showing the planets of our solar system: Mercury, Venus, Earth with its Moon, Mars, Jupiter, Saturn, Uranus, and Neptune. Each planet is shown to scale relative to the others.
Historical astronomical symbols for the planets Ceres and Pallas from 1802.
Animation showing the orbit path of the asteroid Pallas in our solar system.
An image of the asteroid 2 Pallas captured by the Hubble Space Telescope in 2007.

Related articles

This article is a child-friendly adaptation of the Wikipedia article on 2 Pallas, available under CC BY-SA 4.0.

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