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Starts With A Bang

Throwback Thursday: Don’t Forget Vesta!

Before NASA’s Dawn spacecraft found white weirdness on Ceres, it had a close encounter with the second largest asteroid: Vesta.

“I have announced this star as a comet, but since it is not accompanied by any nebulosity and, further, since its movement is so slow and rather uniform, it has occurred to me several times that it might be something better than a comet. But I have been careful not to advance this supposition to the public.” –Giuseppe Piazzi, discoverer of Ceres, the first Asteroid

Out beyond Mars, but not quite out as far as Jupiter, a collection of thousands of rocky objects, ranging in size from pebbles all the way up to the size of Texas, lies the asteroid belt.

Image credit: David Minton and Renu Malhotra.

While the very first asteroid was discovered way back in 1801, with many thinking it was a planet, it was quickly discovered that there were many small, sub-planet-sized objects in between Mars and Jupiter.

Image credit: wikimedia commons users Vystrix Nexoth.

By 1849, there were 10 objects known, with the largest being Ceres and the second largest — at least in terms of mass — being Vesta. As even Ceres is minuscule compared with our Moon (shown in grey, above), none of these objects could rightfully be considered planets, and hence we now consider the entire collection to be the asteroid belt. While the combined mass of every asteroid is just 4% the mass of our Moon, the two largest members, Ceres and Vesta, are on their own estimated to make up nearly 40% of the mass of the entire belt.

Image credit: NASA, ESA, L.McFadden, J.Y.Li (UMCP), M.Mutchler, Z.Levay (STScI), P.Thomas (Cornell), J.Parker, E.Young (SwRI), C.Russell, B.Schmidt (UCLA).

Because of their small sizes and their incredible distance from us, even these two most massive asteroids — about the size of Texas and Arizona, respectively — barely have any discernible features, even when imaged with the Hubble Space Telescope, as shown above.

But these asteroids are very different from our Solar System’s other rocky worlds. For instance, they’re made up of different elements than we are, their surfaces are very, very old, and they’re the closest things we have lying around to protoplanets: the building blocks of our Solar System’s rocky worlds that haven’t been a part of the inner Solar System in over 4 billion years.

Image credit: H. Chang from National Tsing Hua University in Taiwan.

But they are still around in the asteroid belt; Ceres and Vesta are, officially, protoplanets that failed to coalesce into full-on planets. So if we wanted to learn more about the formation of rocky planets in the Universe, that would be the ideal place for a mission.

And — wouldn’t you know — we’ve got just such a mission going on right now: say hello to the Dawn Spacecraft!

Image credit: NASA.

For over a year, from 2011–2012, Dawn was in orbit around Vesta, taking more than 28,000 images, mapping the surface in 3-D, and learning more about this distant protoplanet than any such object ever before. Just a visual comparison of Dawn’s true-color composite of Vesta with the one from Hubble should stop you in your tracks.

Images credit — Dawn view: NASA / JPL / UCLA / MPS / DLR / IDA / color composite by Daniel Macháček; Hubble view: NASA / ESA / STScI / UMd.

While Ceres gets all the headlines these days due to its mysterious white spots, it’s important to remember that Ceres is the second asteroid to be visited, orbited and mapped by Dawn: Vesta came first!

There are some amazing features we’ve found on heavily-bombarded Vesta, some of which are completely unique — as far as we know — to our Solar System. Perhaps the most striking is the impact basin over 300 miles (500 km) in diameter on its South Pole, with a mountain over 14 miles high in the center!

Image credit: NASA / JPL / UCLA / MPS / DLR / IDA.

Known as Rheasilvia — named after the mother of Remus and Romulus — this crater is 90% the diameter of the entire asteroid, and the wave-like ripples you can see throughout Vesta clearly originated from this impact! Perhaps only two or three other asteroids in the entire belt would have survived an impact like this; all others would have been destroyed.

A false-color topographic map that I’ve managed to track down should really show you just how gigantic this feature is.

Image credit: NASA / JPL-Caltech / UCLA / MPS / DLR / IDA.

The impact responsible for this also happened relatively late in the Solar System’s history: while most protoplanetary collisions were done more than 4 billion years ago, Dawn discovered that this impact on Vesta happened just 1-to-2 billion years ago, which is very late for the Solar System.

The great impact also created this remarkable system of trenches along Vesta’s equator, just as “ripples in water” happen when you drop a pebble into a lake.

Image credit: NASA / JPL / UCLA / MPS / DLR / IDA.

These equatorial trenches are many hundreds of kilometers long, which is gigantic considering the entire asteroid is only some 530 km in diameter! You may also notice that, in addition to the normal light-and-shadows you see over the terrain, there are lots of materials on Vesta that are simply intrinsically dark. You can really see this if you look at the “Snowman” on Vesta.

Image credit: NASA / JPL / UCLA / MPS / DLR / IDA.

So while Ceres has its light material mystery, Vesta has a counterpart mystery of its own: where did this dark material come from? One leading theory is that it came from beneath the surface, and was kicked up unevenly by the impact that created Rheasilvia.

What’s kind of remarkable is that tiny “Vestoids”, or rocks originating from Vesta, were undoubtedly kicked off of the giant asteroid from that impact, and some of them made it to Earth! But back to these three “snowman” craters — Marcia, Calpurnia, and Minucia — we’ve got a true-color image of their interiors as well, and they… well, it’s simply remarkable.

Image credit: NASA / JPL / UCLA / MPS / DLR / IDA.

Vesta itself is quite rare in many ways: it rotates very rapidly, completing a rotation in less than 6 hours, and it’s inclined both to the ecliptic (at 7 degrees) and on its axis (at 29 degrees), so that there are no permanently shadowed craters. If we could watch Vesta from afar in space, this might be what we’d see.

Image credit: NASA / JPL-Caltech / UCLA / MPS / DLR / IDA; wikimedia commons user Little Mountain 5.

And while that might strike you as absolutely amazing — and well, it is — it’s still not the most spectacular thing I’ve got to show you. A huge German collaboration has put together this remarkable flyover sequence of Vesta, complete with explanations of what was discovered, and I can’t do it any better justice than the team has already done. (Full info here.)

Three years ago, Dawn departed Vesta and left for Ceres, and is now in the process of mapping and analyzing the Solar System’s largest asteroid. While Vesta may be a distant memory, the science we’ve learned from it is not only going to last us many decades, but is giving us our first opportunity — combined with the Ceres data — to do comparative asteroid studies in situ, and learn just how the bodies that are left over from the young Solar System contributed to the formation of all the planets we know today.

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

This is as close as we’ve ever come to understanding the formation of the Solar System and — by extension — the ultimate origins of everything on our world.

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