Presolar grains inside the Allende meteorite

Illustration of three types of presolar grains inside the Allende meteorite. The grains originated from (left to right) the protosolar system, a nebula and a red giant.
Client
Caltech
Date
January 2020
Categories
Journal Cover Illustration

Project Notes

This illustration was created for a cover submission to Nature Astronomy for Francois Tissot, professor of Geochemistry at Caltech who studies, in part, the formation of the early solar system. The research featured in this image was a study of calcium-aluminum rich inclusions (CAIs), substances found in meteorites that were the first solids to condense in the early solar system. Inside these inclusions are presolar grains, small crystals that actually predate our solar system. By measuring particular isotopes of noble gases in these grains, the researchers can determine where the material in the grain originated – in a red giant, a nebula, or in the protosolar system – and gain insight into the formation of our solar system.

Photo of a fragment of the Allende meteorite.
Photo of a fragment of the Allende meteorite.
Photo of a calcium-aluminum rich inclusion (CAI).
A calcium-aluminum rich inclusion (CAI).

To highlight the different histories of these various presolar grains, we decided to create an image of transparent marble-like grains, each containing its own history of formation.

Image of marbles of various colors.

Here's an early test of these grains, showing the early solar system, a nebula, and a red giant star:

Test render of stylized grains.

The basic idea was to show the meteorite split open, revealing these grains inside:

Sketch of the meteorite split open, spilling grains onto a surface.

However, on an early test render I realized that such a wide view (leaving space for the journal title and additional text) would not highlight the grains properly (after all, they should be the focus of the illustration)...

First test render of the cover.

..so I decided for a closer composition, with three grains embedded in the split meteorite (and some space at the top and bottom left corner for titles):

Zoomed-in version of the cover.

At this point the researchers pointed out that the exterior should be less glossy, more of a rough crust left over from baking in the atmosphere on entry:

Photo of the exterior crust of a fragment of the Allende meteorite.

And that interior surface should also be lighter, with lots of CAIs visible:

Photo of an interior slice of the Allende meteorite, with lots of CAIs visible.

Here's the result of those changes, close to the final version...

Modified version of cover image.

...and here's some close-ups of the new exterior and interior, showing a clear transition between "crust" and interior:

Close-up of the exterior of the meteorite.
The new less-glossy crust.
Close-up of crust and exterior.
Clear difference between crust and interior.

Finally, here's some close-ups of each grain:

The proto-solar grain.
The proto-solar grain.
The nebula grain.
The nebula grain.
The red giant grain.
The red giant grain.

Unfortunately we didn't make the cover, which went to a very deserving review article on blazars (and a lovely cover designed by secondary school students from Padova, Italy.) Before submitting, I made a quick mockup of what the cover might look like if selected: