Have a Happy
Thought:
We live in an
incredible time – a time in which humans are sending robots to literal other
worlds, and bringing back pieces of those worlds to study, back here on Earth.
This has happened
twice now in short succession! Just
last week, a Chinese-led mission returned samples of the “far side” of the
moon back to Earth. This was the Chang-e 6 mission. A couple of things of note
about this mission:
- The
mission name, Chang'e
(嫦娥), is an ancient Chinese
goddess or mythological figure, who lives in/on the moon with her pet
rabbit, which can easily be seen from Earth, in the light and shadows
formed by the highlands and craters visible from Earth.
Image:
the moon as seen through a telescope. Vaughan Turner, supplied.
- While
there is no Dark Side of the Moon, there is a Far Side of the Moon: The
same ‘face’ of the moon always faces the Earth, so different parts of the
moon are lit by the sun as the moon orbits the Earth, and the Earth-moon
system orbit the sun.
- Not only
is this the first time any bits of the far side of the moon have come back
to Earth, China remains the only country to have even landed anything on
the far side of the moon!
- While the
near side of the moon has lots of dark areas, once called mares (oceans)
but we know now they are ancient lava flows, leading to the shapes we
often see, the far side has a lot more craters and few to none of those
mares. No, we don’t know why this is. Yes, we’re hoping that the Chang’e
missions can help solve some of the mysteries here!
Global map of the near and far
sides of the Moon, from NASA’s Clementine spacecraft. Image credit: NASA.
The second recent
sample-return mission was finally completed earlier this year, when a NASA-led
mission returned samples of the asteroid
Bennu. This asteroid probably used to be a part of the asteroid belt
between Mars and Jupiter, but over time this half-kilometre-wide chunk of rock
has drifted closer to Earth, and passes pretty close to us every 6 years.
This mission was
named the Origins, Spectral Interpretation, Resource Identification, and
Security-Regolith Explorer, or OSIRIS-REx for short. It launched from Earth in
2016, collected samples from the asteroid in 2020, and then swung back by Earth
to drop off its payload in October 2023. (The spacecraft is now on its way to
another asteroid to keep exploring).
Between October
2023 and January 2024, engineers and researchers at NASA had to clear one final
hurdle though… or actually two final hurdles: there were 35 fasteners holding
the sample container closed, and two of these just would. not. budge! They
eventually had to develop some extra tools specifically to remove those final
two fasteners, and this
finally worked, after several months of trying!
The great thing
though is that the goal of the mission was to bring 60g of material back to
Earth, and scientists had recovered more than 70g
just from the outside casing – before they even got into that actual sample
container!
Bonus samples 😊 In fact, there was so much bonus material, it
actually took
them even longer to get to those 35 fasteners in the first place.
And just last
week, the team released
images and their initial analysis of these samples… So now you get to see
the beauty of highly-magnified grains of an asteroid.
Examples of coarse-grained
phyllosilicates in sample OREX-501017-0. Image: https://onlinelibrary.wiley.com/doi/10.1111/maps.14227
The really cool
thing is that some of these minerals can also be found at the mid-Atlantic
ridge here on Earth, meaning there may have been a lot of water in and on the
planetoid that Bennu was once a part of.
Examples of magnetite and
sulfide in samples OREX-501001-0, OREX-803079-0, and OREX-501002-0. (a)
Magnetite framboids. (b) Magnetite spheres with radially projecting needles
next to dodecahedral crystals. (c) Dodecahedral magnetite with surface etching.
(d) Magnetite plaquettes. (e, f) Pseudohexagonal plates of pyrrhotites. Image: https://onlinelibrary.wiley.com/doi/10.1111/maps.14227
And they even glow
in UV-light: invite Bennu to your next rave!
Optical and UV fluorescence
imaging. (a) Reflected light image showing the texture and brightness variation
across an aggregate within sample OREX-501006-0. (b) UV fluorescence microscopy
image showing the distribution of carbonates and phosphates (blue fluorescence)
and organic nanoglobules (yellow fluorescence). Image: https://onlinelibrary.wiley.com/doi/10.1111/maps.14227
How can you get
your hands on a bit of asteroid?
Well, if you’re a
scientist you can apply to get a bit
of Bennu for your research.
Or you can find a
meteorite, which has made its own way to Earth. They’re pretty
rare here in Aotearoa New Zealand, but considering they’re found in
deserts, and even rooftops,
you never know what you’ll find once you start looking.
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