Astrophysicist Explains How Earth’s Moon Was Created - Dr David Kipping
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Astrophysicist Dr. David Kipping explores the enduring mystery of how Earth's Moon was formed, centering on the prevailing Giant Impact Hypothesis. This theory posits that early in our solar system's history, a Mars-sized protoplanet named Thea collided with Proto-Earth. Such an impact would have been catastrophic, potentially vaporizing Thea and ejecting massive amounts of material from Earth to form the Moon. While this event explains the origin of the satellite, it presents significant challenges regarding isotopic composition; specifically, lunar rocks collected by Apollo astronauts share nearly identical oxygen isotope ratios with terrestrial rocks, suggesting they formed from the same source material rather than a distinct impactor like Thea leaving its own signature behind. To resolve this discrepancy between theory and evidence, scientists have proposed scenarios such as "Cestia," where the collision was so violent that Earth and the ejected debris merged into a single, rapidly spinning lava donut before separating back into two bodies. This mixing mechanism would allow for homogenization of isotopes while still accounting for the Moon's formation. However, mysteries remain regarding the Moon's physical structure; there is a stark dichotomy between its near side, which features vast smooth plains called Maria formed by ancient lava flows, and the heavily cratered far side with a much thicker crust. Some theories suggest that two moons may have initially formed before one "pancaked" onto the other to create this asymmetry, though these details remain subjects of active debate within the scientific community. The Moon's existence is not merely an astronomical curiosity but a fundamental driver for life on Earth as we know it. Dr. Kipping highlights that the lunar tides helped strip away part of Earth's early thick crust, preventing the formation of a "stagnant lid" similar to Venus and enabling plate tectonics. This geological activity is crucial because it facilitates the carbon cycle; without subduction zones recycling carbon back into the atmosphere as CO2 via volcanoes, life would eventually run out of essential building blocks for growth. Furthermore, the Moon stabilizes Earth's axial tilt (obliquity), ensuring a relatively consistent climate over geologic time scales and creating tidal pools that may have been vital in early evolutionary history. Beyond our own solar system, astronomers are investigating whether such unique events or configurations are common among exoplanets. A key phenomenon discussed is "tidal locking," where an object's rotation slows until it always faces its star with one side, a condition observed on many moons of Jupiter and Saturn as well as close-in planets like Mercury (which orbits in a pseudo-synchronous state rather than being fully locked). While tidal forces generally predict this outcome for bodies near stars, complex factors such as general relativity and planetary composition can alter these dynamics. Current research focuses heavily on the rapid rotation of gas giants like Jupiter and Saturn, which retain their primordial spin because they are too distant from the Sun to be significantly slowed by gravitational braking or magnetic drag. Looking toward future discoveries, Dr. Kipping expresses excitement about upcoming observations using the James Webb Space Telescope scheduled for October. These missions aim to measure the shadows of exoplanets passing in front of other stars with unprecedented precision, allowing scientists to detect subtle bulges caused by rapid rotation and determine tilt angles that were previously unmeasurable. By analyzing these features on a Jupiter analog located over a thousand light-years away, researchers hope to complete the picture of planetary formation processes. This new observational capability will provide critical data on how fast planets spin, their internal composition, and their axial tilts, ultimately helping us understand if Earth's specific history involving its Moon is unique or part of a broader cosmic pattern.
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talking about large impacts can we talk
about the importance of the Moon and its
creation and stuff yeah the the moon's a
puzzle that we still wonder about today
despite the fact it seems like it's a a
sealed story we think the moon formed
from a huge impact it's thought that
there was a mars-sized planet which
smashed into the Proto Earth billions of
years ago for just after the solar
system formed so the Earth would have
been actually been larger then had this
impact not had occurred it would have
been maybe 50% more massive than it is
today maybe twice as massive and this
impactor came along smashed into the
Earth it knocked off a huge amount of
material and it's thought that impactor
which we normally give it the name Thea
would have been almost completely
obliterated in this and vaporized in
this in this collision and then some
chunk of the Earth was knocked off and
that chunk of the earth is ultimately
what formed the Moon or maybe even
multiple moons that then coales later
into a single Moon so there there's a
huge amount of interest about why why
you might come up with a speculative
idea and and still people are
challenging this idea the thing we know
for sure is that the the moon rocks that
were collected by the apoll Apollo
Astronauts have almost the exact same
isotropic ratio of oxygen 18 to oxygen
17 I think it is as Earth rocks do and
this is thought to be a fingerprint that
the rocks formed in the exact same place
around the sun we look at rocks from
Mars we look at rocks from Venus these
are basically meteorites we've collected
that land in on the earth they have
distinct isotropic ratios but the Moon
and the Earth have exactly the same so
that tells us that they formed from the
same inherent clump of
material that's challenging with this
impactor with the impactor if this thing
really did have its own unique origin
this impact to Thea Why didn't it
contaminate
that then and have its own distinct
signature that gets mixed in so that has
been a challenge one idea that has been
suggested to cter this is called cestia
I think I'm pronouncing that right
cestia and that's when the impact
happened it was so uh extreme that it
Formed basically one giant donut-shaped
planet for a while so the Earth and the
moon would have smashed together formed
basically a ball of lava essentially
that was shaped like a almost a donut in
space
spinning very rapidly because of all the
anle momentum from the impact and then
gradually have peeled off and formed a
moon and the earth separately from this
giant impact the reason why this is
attractive because it allows for this
material to mix in come thoroughly so so
this impact to whatever it was Thea and
the Earth completely mix into one single
object and then it separates out into
the Earth and the moon separately that
seems to uh explain some of the
Mysteries but not everybody accepts that
idea and there still a lot of
controversy about the moon like the
moon's Far Side has a very different
appearance and thickness to the near
side if you ever seen a picture of The
Far Side of the Moon it looks radically
different to the near side the near side
has these Maria these beautiful lava
flows that happen millions of billions
of years ago that kind of smooth it out
and then it has these more crated uh
areas whereas The Far Side is almost
completely crated there's very very few
Maria that's because the crust the
actual lithosphere of the moon is much
thicker on The Far Side than the near
side and again that's weird like why why
should that be why is there a dichotomy
like that and so once one idea of there
is that actually Two Moons formed in
this process and then one kind of pancak
onto the back of the the moon today and
that is that pancaking that then formed
like a thicker shell on The Far Side of
the Moon so there's it's like I wish we
had a time machine because this would
have been like the greatest fireworks
shown in in the universe to have seen
the formation of the Moon and again it
raises so many questions like how how
unique was that does that happen in
other exoplant systems are we special
that this happened here we don't really
have any observational evidence either
way but obviously my team and I one of
the things we've been trying to do over
the last few years is to try and detect
moons around other planets to try and
ultimately answer this question because
at the end of the day the moon has a
huge influence on our planet it
stabilizes the obliquity of the earth it
gives us the tides gives us you know the
the rise and the fall of the tides which
potentially are a useful thing for life
they create Rock pools on the on the on
the coastlines especially when the moon
was closer in it would have formed o you
know continent covering Tides basically
the entire continent would have been
covered in a massive tide that would
have formed all these Rock pools all
over the place um it also uh potentially
stripped off the upper mantle the upper
lithosphere of the earth and that could
so basically the crust so the crust may
have been much thicker of the earth when
it first formed and then the impact
could have ripped off some of that thick
crust and had that not had happened the
crust may have been too thick to have
allowed for plate tectonics so plate
tectonics we think are absolutely
crucial for life as light light Life as
we have it on the earth because they
allow for something called the carbon
cycle so when an animal dies in the
bottom of the ocean its carbon is locked
up in its bones and its shell whatever
it is and it settles down to the bottom
of the ocean just stays there and if
there was no if that was just the way it
was the the world would run out of
carbon basically and there'd be no way
for animals to grow on the surface
anymore because there be no carbon left
but instead what happens is these these
plates subduct and they go under each
other and so that carbon recycles it
comes back out in CO2 in volcanoes and
that allows access for photosynthesis to
to happen in plants for instance so
without the carbon cycle it's difficult
to imagine how we'd have the biosphere
we have today and the Moon may actually
be the reason why we have a carbon cycle
for if it had not stripped off that
upper uh that Upper Crust the crust
would have been so thick that would have
formed what we call a stagnant lid a
stagnant lid is what we is seems to be
the case with Venus Venus seems to have
a very thick uh lithosphere which
basically prevents plate tectonics as we
have them on the earth so yeah very
intriguing like you look at all the
things the moon does and you think wow
are we are we a product of the Moon
the idea of plate tectonics kind of
tilling like doing Global tilling uh is
so so fascinating and yeah I I mean the
Moon being tily locked or rotationally
locked what's that what's that called
yeah tily locked yeah tily locked yes so
we only ever see how rare is that to
have something that doesn't rotate at
all that seems bizarre that's pretty
that's actually pretty common so a lot
yeah a lot of meons that's true of
because there and we think we understand
why this should happen whenever you get
fairly close to a planet or a star the
the gravitational effect obviously
increases as you get closer and closer
and it kind of locks in the the shape of
that object to always have one side
facing it so especially if you have some
kind of uh fluids like the Earth does
these Tides can be quite effective
slowing things down um it happens for
many moons around Jupiter Saturn so we
think this is pretty common it's thought
that uh this should be common for
exoplanets as well which is interesting
but again unproven but we think that
there are some Stars which have very
close in planets and those planets are
so close that they should tily lock to
their star and we've measured many of
these hot Jupiters and we've watched
them whiz around their star and we can
even see basically re thermal Maps we
can kind of re thermally map the
distribution of energy on these planets
and they look indeed like they are tidy
locked as you would expect them to be so
everything about exoplant seems to
support this idea that tide locking
should happen but there are also
mysteries of title locking we don't
really know exactly when it stops the
theories of tidal theory that we use are
fairly primitive to be honest they kind
of parameterize things in a very basic
way ideally you would just simulate an
entire planet like every single atom but
we just don't have computers powerful
enough to simulate every single atom so
we use these simplified models and we
know these simplified models don't
always work so for in for mercury it was
predicted that mercury should be tidy
locked to the Sun but it's not it's in a
pseudos synchronous orbit and probably
the reason why that's happening is is
because of general relativity um because
actually there's gen relativistic
effects that come into play when you get
close to a star as well so it's thought
that um TI loocking should happen but in
some instances it's more complicated
than just a simple formula and you
really need to like think about the
composition of the star the composition
of the planet what it's made out of does
it have a core what what's its density
profile like how how much general
relativity kicking in here so the
calculation is quite non-trivial but it
does seem like it's common in the solar
system and expected to be common
elsewhere are there any other
interesting rotations of planets in our
solar
system yeah I mean one of the things I
think is interesting is Uranus uh is
tilted on it side which is like kind of
confusing so even though it's it's spin
isn't particularly unusual it's somehow
been knocked over so it's just spinning
in a sideways config ation so that like
it's rolling forward it's it's like it's
just it's its axis in which it spins
like the Earth's axis is basically
pointed um orthogonal to its to its
orbital plane so normal to its orbital
plane pointing up if you like whereas
for Uranus it's kind of tilted so its
North Pole is pointed at the
sun rolling like it's like it's rolling
forward on a surface that doesn't exist
yeah kind of yeah and and as it as it
goes around what's kind of weird is that
the moons I've also tilted over
alongside it so this has been like
Curious how we can imagine maybe the
planet getting knocked over on its side
but then why are all the moons also on
its side as well we don't really
understand what happened there so very
strange to understand have Uranus and
then one of the one of the cool things
we're thinking about a lot of my team at
the moment in my research group the cool
words lab is the rotation of Jupiter and
Saturn which are rotating pretty fast
once every 10 hours and we think this is
uh to be expected pretty much for all
giant planets once you get far enough
away from the Star so if the if Jupiter
came too close to the Sun that tile
locking thing would cook in and it would
slow Jupiter down it put the brakes on
Jupiter's Spin and slow it down to days
rotation rate basically whatever orbit
period was but Jupiter's far enough away
that it still retains what we would call
its primordial Spin and Jupiter and
Saturn don't really have any way of
getting rid of that spin for the sun it
does loose spin it was probably spinning
much faster when it was young and it's
been losing it through its very strong
magnetic fields Jupiter has magnetic
fields but nowhere near strong enough
that it can lose spin the same way that
the sun does it's so far away from the
Sun that it's not going to be slowed
down by being closer yes correct so it
doesn't really have any way to shed this
spin that's interesting because we are
now we have some observations coming up
with the James web Space Telescope in
October where we're going to basically
measure a Jupiter analog so a planet an
exoplanet around a different it's over a
thousand light years away but we're
going to measure very precisely its
shadow as it passes in front of another
star and we think that this planet
should have simly a fast Spin and why
that's interesting is that that fast
spin causes Jupiter to bulge out at its
equator more than its pole so it's
actually 5% wider than it is tall and
Saturn's 10% wider than it is tall
through this spinning effect we think we
can measure this it's never been
measured before if we can measure it it
will tell us basically what the plet is
made out of how fast it's spinning and
even its tilt angle so as I said Uranus
is tilted right over Jupiter and Saturn
are not very tilted compared to that but
we should be able to actually measure
that angle for the first time and really
get a deeper insight as to how these
plants are forming so I'm just excited
that we might have access for the first
time thanks to James web to a completely
new observational technique learning
about exoplant we have their Mass we
have their radius but now we can get
their spin their bulgin their their tilt
angle and really just complete the
picture as to how these things formed
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