Locals watched in awe as a fireball exploded and hundreds of meteorite fragments rained down on the city of Tatahouine, Tunisia, on June 27, 1931. Fittingly, the city later became a major filming location of the Star Wars movie series. The desert climate and traditional villages became a huge inspiration to the director, George Lucas, who proceeded to name the fictional home planet of Luke Skywalker and Darth Vader “Tatooine”.
The mysterious 1931 meteorite, a rare type of achondrite (a meteorite that has experienced melting) known as a diogenite, is obviously not a fragment of Skywalker’s home planet. But it was similarly named after the city of Tatahouine. Now, a recent study has gleaned important insights into the the origin of the meteorite – and the early Solar System.
Lucas filmed various scenes for Star Wars in Tatahouine. These include Episode IV – A New Hope (1977), Star Wars: Episode I – The Phantom Menace (1999) and Star Wars: Episode 2 – Attack of the Clones (2002). Various famous scenes were filmed there, including scenes of “Mos Espa” and “Mos Eisley Cantina”.
Mark Hamill, the actor who played Luke Skywalker, reminisced about filming in Tunisia and discussed it with Empire Magazine: “If you could get into your own mind, shut out the crew and look at the horizon, you really felt like you were transported to another world”.
Composition and origin
Diogenites, named after the Greek philosopher Diogenes, are igneous meteorites (rocks that have solidified from lava or magma). They formed at depth within an asteroid and cooled slowly, resulting in the formation of relatively large crystals.
Tatahouine is no exception, containing crystals as big as 5mm with black veins cutting cross the sample throughout. The black veins are called shock-induced impact melt veins, and are a result of high temperatures and pressures caused by a projectile smashing into the surface of the meteorite’s parent body.
The presence of these veins and the structure of the grains of pyroxene (minerals containing calcium, magnesium, iron, and aluminum) suggest the sample has experienced pressures of up to 25 gigapascals (GPa) of pressure. To put that into perspective, the pressure at the bottom of the Mariana Trench, the deepest part of our ocean, is only 0.1 GPa. So it is safe to say this sample has experienced a pretty hefty impact.
By evaluating the spectrum (light reflecting off their surface, broken down by wavelength) of meteorites and comparing it to asteroids and planets in our Solar System, it has been suggested that diogenites, including Tatahouine, originate from the second largest asteroid in our asteroid belt, known as 4 Vesta.
This asteroid possesses interesting and exciting information about the early Solar System. Many of the meteorites from 4 Vesta are ancient, around ~4 billion years. Therefore, they offer a window to the past events of the early Solar System that we are unable to evaluate here on Earth.
By combining the age dating techniques and the microscope technique, the authors managed to map the timing of impact events on 4 Vesta and the early Solar System. The study suggests that 4 Vesta experienced ongoing impact events until 3.4 billion years ago when a catastrophic one occurred.
This catastrophic event, possibly another colliding asteroid, resulted in multiple smaller rubble pile asteroids being produced known as “vestoids”. Unravelling large scale impact events such as this, reveals the hostile nature of the early Solar System.
These smaller bodies experienced further collisions that caused material to hurtle to Earth over the last 50 to 60 million years – including the fireball in Tunisia.
Ultimately, this work demonstrates the importance of investigating meteorites – impacts have played a major role in the evolution of asteroids in our Solar System.
Post a Comment