Sky & Telescope - May 2020 - 4

SPECTRUM

by Peter Tyson

A Vote for Motes

The Essential Guide to Astronomy
Founded in 1941 by Charles A. Federer, Jr.
and Helen Spence Federer

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4

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EDITORIAL
Editor in Chief Peter Tyson
Senior Editors J. Kelly Beatty, Alan M. MacRobert
Science Editor Camille M. Carlisle
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Associate Editor Sean Walker
Observing Editor Diana Hannikainen
Consulting Editor Gary Seronik
Editorial Assistant Sabrina Garvin
Senior Contributing Editors
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Contributing Editors
Howard Banich, Jim Bell, Trudy Bell, John E. Bortle,
Greg Bryant, Thomas A. Dobbins, Alan Dyer,
Tom Field, Tony Flanders, Ted Forte, Sue French,
Steve Gottlieb, David Grinspoon, Shannon Hall,
Ken Hewitt-White, Johnny Horne, Bob King,
Emily Lakdawalla, Rod Mollise, James Mullaney,
Donald W. Olson, Jerry Oltion, Joe Rao, Dean Regas,
Fred Schaaf, Govert Schilling, William Sheehan,
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Charles A. Wood
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toss around a certain astronomical term without thinking much
about it: dust. "Interstellar clouds of gas and dust," we'll say, or
"Check out that galaxy's dust lane, will you?" But in light of several articles in this issue, it's worth pausing to consider just what
astronomers mean by dust and how much we owe to it.
Cosmic dust comes in many sizes and flavors. It all starts with those chemical building blocks, elements such as carbon or silicon. When interstellar particles with such elements at their core grow too large to be called molecules -
when, through collision, aggregation, and other processes, they reach umpteen
millions of atoms - we start calling them dust. We're still talking tiny: only up
to micron-size, or one-millionth of a meter (0.000039 inch). By comparison, a
droplet of water in fog is about 10 microns in diameter; a strand of spider silk is
3 to 8 microns across.
Bits of cosmic dust stick together, of course. When a particle reaches a size
you could see if it were perched on your fingertip, we often label it a pebble.
After all, these centimeter-size grains are, in essence,
minuscule rocks. That's what you see shooting out
of the asteroid Bennu in the photo on page 20. In
her article on protoplanetary disks (page 34), Megan
Ansdell describes how astronomers use the ALMA
radio-telescope array to study pebble-size dust and
the SPHERE instrument to analyze micron-size dust,
which she likens to smoke.
Hubble close-up of the
Then there's the dust that grows so large you could
Horsehead Nebula
stand on it (see cover). It's arresting to think that our
very Earth, as all planets, arose from motes: particles to pebbles to planetesimal
to planet. Did our vast world really begin as mere specks? It had to start somewhere, and just as we might follow a mighty river back to its source in a hillside
spring, could we, if we had a time machine, trace our globe back to grains?
Back to Earth: As all astronomers know, dust enables us to see and learn
from wonders of the night sky that might otherwise remain invisible to us.
Supernova remnants. Meteor showers. The zodiacal light. Star-blocking clouds
like the Coalsack. Star-forming regions like the Orion Nebula. Dust storms on
Mars. The tails of comets (page 41). Want to add your own examples?
Then there's the fact that we're all stardust, as Carl Sagan reminded us. Every
atom in our bodies, save for atoms of hydrogen and one or two of the other
lightest elements, was forged in stars billions of years ago.
So let's give a nod to cosmic dust. It's us.

AMERICAN ASTRONOMICAL
SOCIETY
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State University
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Kelle Cruz, CUNY Hunter College & AMNH;
Kelsey Johnson, University of Virginia
At-Large Trustees Tereasa Brainerd, Boston University;
Hannah Jang-Condell, University of Wyoming

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Sky & Telescope - May 2020

Table of Contents for the Digital Edition of Sky & Telescope - May 2020

Contents
Sky & Telescope - May 2020 - Cover1
Sky & Telescope - May 2020 - Cover2
Sky & Telescope - May 2020 - 1
Sky & Telescope - May 2020 - Contents
Sky & Telescope - May 2020 - 3
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