Ida and Dactyl

Galileo Probe image from NASA

Typically, asteroids are too small to have their own satellites. The gravitational force exerted by an asteroid is too minor to hold on to any object larger than a boulder if that object passes close by. The object are moving faster than the escape velocity of the asteroid. However, there are exceptions. The prime example is the dual system of Ida and Dactyl.

243 Ida was the 243rd asteroid discovered in the Asteroid Belt. It was originally discovered by Austrian astronomer Johann Palisa in 1884. Based on the spectroscopy, Ida is an S-type asteroid with an albedo of 0.2383. It has a semi-major axis of 2.862 AU, taking 4.84 Earth years to orbit the Sun. It has an average diameter 31.4 km across which is kinda weird to use since it is longer than it is wide.

In 1993, the space probe Galileo visited Ida on its way to explore Jupiter. It was in this visit where Dactyl was discovered. Dactyl is only 1/20th the size of Ida, only about 1.4 km in diameter. It is difficult to determine Dactyl's orbital characteristics without much more observation, but because it is so small in relation to Ida, to determine how it orbits Ida, Dactyl and Ida will have to be visited. Constraints to its orbit did allow a density to be roughly detemined and Dactyl is lacking metallic minerals. Ida and Dactyl share similar characteristics, so it is possible that they formed at the same time.

1 Ceres

NASA's Solar System Explorations Page



Ceres was the first asteroid discovered in the Asteroid Belt on 1 January 1801 by Giuseppe Piazzi. When he first discovered it, he thought it was a planet, as it was a common belief at the time that there might be a planet between Mars and Jupiter because of the large gap between the two planets.
Because there was not enough information to determine the orbit of Ceres, it wasn't confirmed to exist until December of 1801. After close observation of Ceres, it was determined that it was not a planet, but something new. It was then that William Herschel coined the term "asteroid" as the object had a star-like appearance so was difficult to distinguish from the background stars. However, after observing Ceres and other asteroids over the course of days and weeks, it was apparent that asteroids move faster in the sky than the stars since they are much closer to Earth.

Ceres is small compared to the planets and many satellites, but it is the largest object in the Asteroid Belt by a wide margin. 

• It has a diameter of about 950 km or the size of Texas
• It's mass is 9.47x10²° kg, or about 0.00016% of the Earth. Despite its mass, Ceres contains 25% of all the mass in the Asteroid Belt
• It has a semi-major axis (orbital radius) of 2.76 AU

As shown in the opening picture, Ceres is relative spherical. Much like the planets, is an oblate spheroid with a wider diameter at the equator than the poles. This shows that it rotates on an axis uniformly. Other asteroids with irregular shapes kinda tumble and wobble in space as they rotate.

We've learned more about Ceres as telescopic observations became more sophisticated and advanced. Ceres does not fit into the three main types of asteroids mentioned in the previous post. In fact, like planets, it is differentiated (layered) with a rocky core, an icy mantel, and an outer crust.

NASA's Solar System Explorations Page

For the next two centuries, Ceres was still considered an asteroid as there was no other category of object it fit in. It's official designation was 1 Ceres as it was the first asteroid discovered and Ceres is its proper name. However, in 2006 when Pluto was demoted from planet status to minor planet, it was concluded that Ceres should be upgraded. Ceres is now officially considered a dwarf planet. It is too small to be a planet (and where the lower limit to be considered a planet is still murky) but too large and too regularly shaped to be an asteroid.

One final weird thing discovered on Ceres is that it is slightly active. An object as small as Ceres should not have any sort of eruptions going on, but in January of 2014, the Herschel Space Telescope discovered water vapor plumes emitted from the surface. We will learn more about Ceres in the coming years when the space probe Dawn arrives at Ceres and begins its exploration. Ceres is also the third most likely spot for crewed missions to visit after the Moon and Mars.

Asteroids

Asteroids are believed to be remnants from the formation of the Solar System. The majority of these objects are found in the space between Mars and Jupiter called the asteroid belt.



As seen in the above image, there are also a few asteroids that are 60° ahead of Jupiter called "Greek" asteroids and some that are 60° behind Jupiter called "Trojan" asteroids. Not seen, but will be discussed are the three-A asteroid groups: Amor, Apollo, and Aten. These are near-Earth asteroids that are a concern for scientists and are searched for and catalogued by astronomers.

In our previous post about Phobos and Deimos, we learned a little about C-type and D-type asteroids. There are two other main types (and no, they are not A-type and B-type) called S-type and M-type. As mentioned before, C-type asteroids (and to an extent, D-type) have strong carbon lines in their spectra. S-type asteroid are stony asteroids, made of silicates, with densities similar to Earth's density, and make up about 17% of all asteroids. M-type asteroids are metallic, with the most common metal found in them iron and some having nickel. This is one reason why mining asteroids might be a lucrative business in the future, when travelling easily from Earth to the outer reaches of the Solar System will be achieved.

253 Mathilde - C-type Asteroid

NASA

15 Eunomia - S-type Asteroid

Astronomical Institute of the Charles University

16 Psyche - M-type Asteroid

Astronomical Institute of the Charles University

 



 Asteroids, generally, come in many sizes, with the largest being 1 Ceres at 950 km in diameter. However, most asteroids are only a few miles in size and are irregularly shaped. It is typically believed that asteroids are planetessimals (baby planets) that were not able to accrete into a planet because of the presence of Jupiter. Measurements of the mass of the asteroid belt show that there is only enough mass there to create a planet with the quarter of the size of a planet.

Asteroids have two parts to their names, a number designation and a proper name. The first few asteroids were just given names, but as more and more were discovered, astronomers started placing a number in front to give an indication of the sequence of discovery. So 1 Ceres was the first asteroid discoved and 253 Mathilde was the 253rd. As of 2013, there are several hundred thousand asteroids named with more than a million probably out there. Many of those asteroids are in the asteroid belt, but as mentioned above, there are thousands leading and trailing Jupiter in its orbit and thousands that are near Earth's orbit. We will learn more about Amor, Aten, and Apollo asteroids in a future post.

Most asteroids orbit independently around the Sun, but there are some that mutually orbit each other.  The most well known pair is Ida and Dactyl, where Dactyl was the first satellite discovered around an asteroid.  The Solar System is a strange place.