Transcript Document

Formation of Mercury
By Triana Henz
In the beginning…
• There was a giant cloud of particles within
the Milky Way
• Particles start to rotate
• The cloud starts to collapse on itself
• A star is born at the center!!
What takes place in a few Myr?
• Accretion Theory takes place
• Heavy elements make their way closer to
the sun
• A temperature difference takes place at
about 4 AU, allowing the inner gas to be
hotter
Planets
• Particles gather to form cosmic dust
• Cosmic dust stick together to grow into
small planet like objects
• The small planet like objects collide with
each other
• As the dust clears, we have proto-planets!!
Mercury
• The out-liner of the
inner planets
• Has a high
density, molten
core, magnetic
field, and a big
core
Thoughts on the mysteries
• Theories have to
account mostly for the
high density that is
observed
• Most theories take
place during the early
stages of the solar
system
• Three leading
theories:
– Selective Accretion
– Post-accretional
vaporization
– Giant impact Stripping
Selective Accretion
• Enrichment of iron that leads to the
high density
• Principles:
– Needs mechanical and aerodynamic
accretion processes
– A low chemical equilibrium
condensation temperature
Why was iron so rich?
• The solar nebula in the feeding zone was
naturally rich with iron
• Particles were so close to the Sun that it
was reducing the other elements to a
metallic form that had a high melting point
to solidify
• This process could explain why Mercury is
highly density
Post-accretional Vaporization
• After Mercury was formed, the solar winds
were strong enough to blow away the
original surface
• The solar winds would’ve contained
intense solar electromagnetic and particle
radiation
Giant Impact Stripping
• Object crashed into Mercury
• Object needs to be about Mars size
• The impact had blown away the upper
layers of proto-Mercury
Correct Theory?
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Depending on when Mercury was impacted, the material ejected would
need to go somewhere
Candidates for where the material ended up are the Sun, Venus, and Earth
The Solar Winds would most likely leave a few traces of the proto layers
since the Solar Winds wouldn’t be able to make a near spherical object
Chemical equilibrium condensation models for the solar nebula can’t
account for a molten core at Mercury’s present orbit or density if formed
between .4-1.4 AU
The condensation models also need to take into account why Mercury is the
only one that is affected by the lower temperature
To know which of the theories is correct, chemical composition needs to be
known of the surface
Each would leave trace evidence of their existence since each has their
own unique signature of oxides and iron oxides
One More Thing…
• There is no doubt that the position of
Mercury gives itself to an unique formation
• It has us believing that we’ll know our solar
system and all planet formation if we study
it closely
• And now we look