Showing posts with label space. Show all posts
Showing posts with label space. Show all posts

2016-10-04

Tomanowos - the rock that went through cosmic billiard, megafloods, and idiocy

Present display of the meteorite at the AMNH museum in NY. My photo.
Last week I visited again the rock with the most fascinating story on Earth: 
Tomanowos, meaning the visitor from the sky in the extinct Clackamas language, also known as the Willamette meteorite. 
Supernovas spread throughout space the
iron produced in heavy stars. This ejected iron
ends up in particle nebulas that eventually form
new stars and protoplanets. [Image: NASA] 

When European Americans found it near the Willamette River (Portland, OR) more than a century ago, Tomanowos inevitably went through one of the most hilarious and silly geological stories that I know of, surely driven by the fatal attraction that a rare rock like this exerts on humans. But before going into that let me tell a few things about its origins.

Tomanowos is a rare 15 ton meteorite made of iron and nickel (Fe 91%, Ni 7.6%). As in other metal meteorites, these Fe and Ni atoms formed at the core of stars that shattered the space with the products of nuclear fusion when ending their lives in supernovae explosions. These elements ended up in the nebula that clumped together as protoplanets in our Solar System, and Tomanowos was part of the core of one of these protoplanets, where the heavier metals accumulate. 

Vesta, a surviving protoplanet of the 
early Solar System. Due to their large
 size, protoplanets develop a differenciated 
density distribution with heavier elements like 
iron concentrated in the core. Tomanowos is an 
ejected piece of a protoplanet core like this. 
[EPFL/Jamani Caillet, Harold Clenet]
We also know that later on, about 4 billion years ago, a collision between two of those protoplanets sent our museum piece back to space solitude. Subsequent impacts over billions of years eventually made the orbit of this meteorite cross that of the Earth. As a result of such cosmic billiard, the meteorite entered our atmosphere at a speed of ~60,000 km/h nearly 20,000 years ago and landed on an ice cap in Canada.

Over the following decades, the ice flow slowly transported Tomanowos southwards, towards a glacier lobe that was at the time blocking the Fork River in Montana (USA). The glacial tongue piled ice across the river valley forming a 600-m-high ice-dam that impounded the enormous Lake Missoula. Following the ice flow, Tomanowos happened to reach the dam on the precise year when it collapsed, releasing one of the largest floods ever documented: the #MissoulaFloods that shaped the Scablands in Washington. This process is known as glacial outburst flooding and it still happens every few years in the Perito Moreno glaciar, for example. Except that the water discharge during the Missoula Floods reached the equivalent to a few thousand Niagara Falls. The research of the Missoula floods by Bretz and Pardee in the early 20th century led to one of the most significant paradigm shifts in recent geoscience: the recognition that catastrophic events can significantly contribute to the evolution of  landscape.
Map of the Missoula Floods path, showing Lake Missoula 
(blue), the ice cap where Tomanowos landed (north of the 
lake outlet), and the inundated areas of Washington and 
Oregon (grey).
Source: Washington Univ.

Trapped in ice and rafted down by the flood, Tomanowos crossed Idaho, Washington and Oregon along the overflown Columbia River at speeds sometimes faster than 20 meters per second. While floating up on the flood waters near today's Portland, the ice case broke apart and the meteorite sunk in the flooding waters. Hundreds of other ice-rafted erratics (rocks that do not match the local geology, nor could be transported by rivers or glaciers) have been found along the Columbia River. All are souvenirs from the Missoula floods, but none as rare as Tomanowos.

As the flood ceased, the sunk meteorite became exposed to the atmosphere. Over thousands of years, rain mixed with the iron sulfide inclusions producing sulfuric acid that gradually dissolved the iron of the exposed side of the rock:
These cavities were produced by acid dissolution of iron at the exposed side.
A few thousand years after the flood, the Clackamas arrived to Oregon and named the meteorite as the Visitor of the Sky, a heaven's representative that unified earth, water & sky. Apparently they knew that nickel rocks come from heaven. Were they intrigued by the absence of a crater at the Meteorite site? In any case, the name reminds us that pre-scientific cultures were not idiotic, or not more than us today anyway.

To confirm this latter hypothesis, in 1902 a colonist named Ellis Hughes decided to secretly move the iron rock to his own land and then claim property. Millennia of peaceful rest in the Willamette valley had to come to an end. But because moving a 15-ton rock a distance of 1,200 m without being noticed is not easy, not even in Oregon, Hughes and his son labored for three back-breaking months in secrecy: 

As D. J. Preston hilariously explains, after finally
succeeding with the moving, Hughes built a shack around
the meteorite, announced he had found it on his property
and started charging twenty-five cents admission to view
the heavenly visitor.
It was during this transport that the rock sadly underwent severe mutilations.
Unimpressed by this deployment of idiocy, Hughes' neighbor fabricated a lawsuit contending that the meteorite had, in fact, landed on HIS property. And to buttress his case he showed investigators a huge crater on his land. The case was dismissed when a third neighbor reported a great deal of blasting only the week before the trial.

Ironically, the legitimate owner of the original land of the iron rock turned out to be the Oregon Iron and Steel Company, so far unaware of the meteorite but promptly hiring a twenty-four-hour guard who sat on top of it with a loaded gun while the case was being appealed. They won the case in 1905, selling Tomanowos to the AMNH museum in New York a year later.
Tomanowos in the early 1900s, before being transported to the AMNH.

Today, amazingly enough, the AMNH exhibition does not even mention the Missoula Floods as a key part of Tomanowos' story, in spite of the wide scientific consensus. Same as the meteorite, the Clackamas were also reallocated to a reservation. Their descendants do keep the right to visit Tomanowos in NY and talk to the visitor who brought the Sky, the Water, and the Earth together.

2014-08-18

67P - how much is a comet worth

I've been trying to learn a bit more about comets (call it summer-research) taking the chance of the visit of the ESA Rosetta mission to comet 67P (aka Churyumov–Gerasimenko).

Comets are small bodies of rock and ice thought to form in the outer regions of the solar system at the same time planets were formed, ca. 4.6 billion years ago. An important known unknown about comets is their relative contribution to the accumulation of water in the early Earth. So learning about them is learning about our planet too.

67P is a 4 km-long ice body orbiting around the sun every 6 years, following an elliptical orbit ranging between those of the Earth and Jupiter.
Barcelona and 67P, to scale
The shape of 67P suggests that it might be the result of the accretion of smaller comets. In fact, one thing that surprises many of us who are unfamiliar with comets is their low density. Most of the comet you see in these pictures has been left empty during its formation. 67P is about 10 2.5 times lighter than water: 102 400 kg/m3 (figures updated after Rosetta's approach), implying that it is a very porous body. Is this related to an accretion process?
Image taken on 2014-08-12 from a distance of 103 km. Credit: ESA/Rosetta/NAVCAM

Another curious fact: 67P used to have a perihelion distance of 2.7 AU (1 AU = distance from the Sun to the Earth), but in February 1959 an approach to Jupiter reduced this to only 1.3 AU, where it remains today. Comets are often shifted by the gravity field of planets, but recent events like this remind us that we are not in a static Solar System. The same process can lead to the split of comets in pieces: a beautiful example is given by the comets 42P/Neujmin and 53P/Van Biesbroeck, which appear to be fragments of a parent comet. This is based on computer integration, a reconstruction of their past position, showing that both comets were close to Jupiter in January 1850 and had nearly identical orbits before that. The debris produced by such comet disintegrations is often responsible for meteor showers like the Perseids seen worldwide in middle August.
Approach to a distance of 104 km.
67P rotates once every 12.7 hours.
Credit: 
ESA/Rosetta/NAVCAM

Rosetta's won't be the first mission actually touching down on a comet (check this list of space missions that have approached comets, and see the unsubtle 'landing' of Deep Impact in the animation below). But it is the first mission ever to smoothly land on a comet (Philae lander) and to analyze its surface. And it is the first mission to orbit a comet, something remarkable since the escape velocity of 67P is only 0.5 m/s. It will also be the first mission to land a probe on the surface and, in the words of ESA, Rosetta will be "the first spacecraft to fly alongside a comet as it heads towards the inner Solar System, watching how a frozen comet is transformed by the warmth of the Sun". A lander will sample the composition and structure of the comet nucleus, drilling more than 20 cm into the subsurface for analysis at the onboard laboratory. 

Rosetta has costed the europeans around 1 billion euros (10^9 €) through a consortium of the German Aerospace Research Institute (DLR) with ESA, CNES, and european and american research institutes. The results will provide information on how comets form and also on the early stages of the Solar System. It should contribute to the discussion on where did the terrestrial water form and when did it arrive here. Previous studies have shown that the isotope ratios of hydrogen in other comets is different from that of oceanic water, but it remains unclear that these comets were representative enough of the comet orbits most likely to contribute to our waters. New answers will arrive soon, together with new questions. 

Deep Impact colliding with comet Temple 1 in 2005