[meteorite-list] Mercury Shrinking More Than Thought

From: Ron Baalke <baalke_at_meteoritecentral.com>
Date: Mon, 9 Dec 2013 18:07:23 -0800 (PST)
Message-ID: <201312100207.rBA27NI7002321_at_zagami.jpl.nasa.gov>


Mercury shrinking more than thought
Latest views of the planet settle a decades-old argument about its evolution.
Alexandra Witze
09 December 2013

The planet closest to the Sun has shrivelled much more over its lifetime
than previously thought, scientists have found.

Studies of Mercury show that it has shrunk by about 11 kilometres across
since the Solar System's fiery birth 4.5 billion years ago. As the planet
cooled and contracted, it became scarred with long curved ridges similar
to the wrinkles on a rotting apple.

A new census of these ridges, called lobate scarps, has found more of
them, with steeper faces, than ever before. The discovery suggests that
Mercury shrank by far more than the previous estimate of 2-3 kilometres,
says Paul Byrne, a planetary scientist at the Carnegie Institution for
Science in Washington DC. He presented the results today at a meeting
of the American Geophysical Union in San Francisco, California.

The finding helps explain how Mercury's huge metallic core cooled off
over time. It may also finally reconcile theoretical scientists, who had
predicted a lot of shrinkage, with observers who had not found evidence
of that - until now. "We are resolving a four-decades-old conflict here,"
Byrne told the meeting.

Planetary scientists have been arguing over Mercury's lobate scarps ever
since the Mariner 10 spacecraft flew past the planet three times in 1974-75.
Researchers can use measurements of the length and height of the scarps
to calculate how much planetary shrinkage they represent.

That shrinkage is a product of Mercury's odd composition - "like a core
floating through space with a thin outer blanket," says Byrne. Most of
the planet is made of that large core, and so it would have cooled rapidly
as heat rushed toward its surface. Modelling studies have long suggested
that the planet should have shrunk by 10-20 kilometres over its lifetime,
compared to the 2-3 kilometres estimated from Mariner 10 data1.

The latest estimates come from NASA's MESSENGER probe, which photographs
and measures Mercury's topography. Last year, Italian scientists used
MESSENGER data covering one-fifth of the planet to show that its shrinkage
was probably greater than the Mariner 10 estimates2.

The latest work, covering the entire planet, revealed many lobate scarps
with sharp vertical relief, Byrne said. It also uncovered details on another
kind of surface feature that may be related to shrinkage. These "wrinkle
ridges" are less pronounced than the lobate scarps but may also have formed
during contraction. Combined, the data on the lobate scarps and the wrinkle
ridges suggest that Mercury's diameter has shrunk by 11.4 kilometres,
Byrne said. Even leaving out the wrinkle ridges gives 10.2 kilometres
of contraction.

Those numbers are plausible to at least one planetary scientist who studied
Mercury's shrinkage using Mariner 10 data in the 1970s. Jay Melosh, a
planetary geologist at Purdue University in West Lafayette, Indiana, suspects
that even more lobate scarps may be lurking out there. "Many of these
things may still be hiding," he says. "As far as I'm concerned, this may
be an underestimate of the amount of shrinkage."



    Dombard, A. J. & Hauck, S. A. Icarus 198, 274???276 (2008).

    Di Achille, G. et al. Icarus 221, 456???460 (2012).
Received on Mon 09 Dec 2013 09:07:23 PM PST

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