Bay Area Skeptics

The San Francisco Bay Area's skeptical organization since 1982

The SciSchmooze

Lili Galillean
14 September 2026


Greetings, fellow carbon-based stargazers!

In introductory astronomy, we are taught a tidy, comforting binary about the debris circling our Sun:

  • Asteroids are dry, rocky, metallic rubble forged in the warm inner solar system inside the “frost line.”
  • Comets are dirty snowballs—fragile agglomerations of volatile water ice, frozen gases, and dust preserved in the deep freeze of the outer Solar System.

It’s an elegant classification scheme. It is also an oversimplification that modern planetary science is actively dismantling.

When you look closely at the architecture of our Solar System, the line separating asteroid from comet isn’t a hard boundary; it is an active spectrum of volatile depletion, thermal baking, and violent gravitational migration. Planetary systems do not form in static, orderly rings—they violently reshuffle their cards, tossing icy outer bodies inward and scattering rocky fragments outward.

This week, we explore the dynamic reality of cosmic debris: stepping from hypervelocity cometary dust incinerating in our upper atmosphere to ancient planetesimals locked in gravitational limbo around Jupiter.

Grab your red headlamp and bundle up. It’s time to look at what planetary systems leave behind.


1. The Icy Stream: The Perseids, Pinnacles, and the Citizen-Science Mesh

Every August, Earth barrels through the orbital wake of Comet 109P/Swift-Tuttle at a blistering 59 km/s (133,000 mph). Back in 1992, early orbit-determination models sparked a brief scientific scare when calculations couldn’t rule out an Earth collision on its 2126 return (IAUC 5636). Fortunately, celestial detective work saved the day: by linking modern astrometry to 18th-century Chinese records, astronomers extended the observational baseline and proved the comet will safely miss us by roughly 14 million miles (Marsden et al. 1993). We dodged a planetary-scale impact, but we still collide with the titan’s shed skin every summer, flash-ionizing milligram-sized grains into the incandescent streaks of the Perseid meteor shower.

Field Notes: Midnight Under the Spire at Pinnacles

Though we had missed the shower’s official peak by a couple of nights, yours truly and friends headed out to Pinnacles National Park (East) on the night of August 15th to catch the lingering waning wave of the shower firsthand.

Taking advantage of the moonless skies, the San Jose Astronomical Association (SJAA) partnered with the National Park Service to host a public star party, bringing observers, families, and dark-sky enthusiasts together under the rugged volcanic shadows of the park.

A massive shout-out to the dedicated volunteers and docents of the SJAA for organizing these events! If you are in the Bay Area and want to experience dark-sky observing with passionate amateur astronomers, check out the SJAA Events Calendar.

Stargazing at Pinnacles National Park (East) around midnight on August 15th, catching the Perseids and the faint glow toward Perseus.

Toward the northeast, meteors sliced through the starfields overhead, tracing their trajectories straight back to the radiant in Perseus against the arch of the summer Milky Way.

What stood out just as much was how much amateur astronomy has evolved. The days of freezing over a fogged manual eyepiece are giving way to automated digital observing. Observers set up smart astro-cameras that autonomously tracked celestial coordinates, live-stacking exposures in real time to resolve faint spiral galaxies directly onto iPad displays under red-light discipline.

Live-stacking deep-sky photons: an automated smart camera resolving a spiral galaxy on an iPad display during the SJAA Pinnacles star party.

The Citizen-Science Mesh: The Global Meteor Network

This democratization of imaging technology is also reshaping planetary defense. Beyond local star parties, amateur observers worldwide have joined the Global Meteor Network (GMN).

Using low-cost Raspberry Pi single-board computers paired with sensitive video security sensors and open-source machine vision, this decentralized mesh network monitors the night sky continuously. When multiple stations spot the same meteor streak, the software automatically triangulates its 3D atmospheric trajectory, measures its deceleration, and reconstructs its pre-impact solar orbit.

If you want to contribute to active meteor science from your own roof or backyard, check out the GMN Camera Build & Setup Guide.


2. The Outer Frontier: Lucy, the Trojans, and the Death of the Binary

If comets are defined by volatile venting and luminous dust tails, asteroids are traditionally assumed to be inert, collisional rocks. But as we venture further out, that distinction begins to collapse.

To investigate these primordial building blocks up close, NASA launched the flagship Lucy Mission. Lucy is currently on a 12-year voyage to explore the Trojan asteroids—two massive swarms trapped in Jupiter’s gravitationally stable L4 and L5 Lagrange points, orbiting 60 degrees ahead of and behind the giant planet. For an overview of the mission’s science goals and instrument suite, watch NASA Goddard’s Studying Trojan Asteroids with Lucy.

Even Lucy’s warm-up flyby of the small inner-belt asteroid Dinkinesh in late 2023 proved that small bodies are far from simple, monolithic rocks. The encounter revealed that Dinkinesh is orbited by a tiny companion moonlet, Selam, which turned out to be an exquisite contact binary—two spherical lobes resting gently against each other like an hourglass (narrated by NASA in Lucy Sees Asteroid Dinkinesh in Detail).

Yet the real prize lies further out with the Trojans. Astronomers have found that these bodies don’t look like dry rocks at all; they are dark, reddish objects rich in tholins—complex, tar-like organic polymers formed when solar ultraviolet radiation and cosmic rays irradiate simple compounds like methane and nitrogen—and likely conceal deep reservoirs of subterranean water ice. In essence, many asteroids are simply dormant, baked comets in disguise.

Along with recent discoveries of active asteroids sprouting surprise cometary dust tails in the asteroid belt, the evidence is clear: the Solar System isn’t divided into two rigid filing cabinets, but exists along a dynamic continuum shaped by collision, heating, and time.


The SciSchmooze Skeptical Twist: Resisting the Binary Trap

We humans have a built-in cognitive bias toward binary classifications: inner vs. outer, rocky vs. icy, asteroid vs. comet. It makes cataloging the night sky feel neat and manageable.

Here is our healthy dose of SciSchmooze skepticism: Nature does not care about our textbook taxonomies.

When an icy body from the deep freeze of the outer Solar System gets dragged inward, bakes away its surface volatiles over thousands of orbits, and develops an insulating refractory mantle, does it stop being a comet? When a rocky asteroid in the main belt reveals a trapped pocket of ancient ice and briefly sprouts a tail, does it become one?

Nature doesn’t trade in neat labels. These bodies are planetary castaways—survivors of the same chaotic reshuffling that assembled the world beneath our feet.


Clear skies, dark horizons, and may your automated camera trackers never lose alignment.

Cosmically yours,
Lili


My Top 3 Picks: Bay Area Science Events (Sept 14–21)

  • SETI Institute Colloquium Series
    • When & Where: Wednesday, Sept 16, 2026, 12:00–1:00 PM | Mountain View, CA & YouTube Live
    • Focus: Planetary science, astrochemistry, primitive asteroid volatiles, and biosignature detection.
    • Details: Free public hybrid lecture featuring visiting researchers, followed by a live 15-minute audience Q&A.
    • Link: SETI Institute Colloquia
  • UC Berkeley Astronomy Department Colloquium
    • When & Where: Thursday, Sept 17, 2026, 3:45–5:00 PM | 131 Campbell Hall, UC Berkeley
    • Focus: Galaxy formation and evolution, the circumgalactic medium, and observational astrophysics.
    • Details: Departmental lecture featuring Prof. Alice Shapley (UCLA); open to visitors, with tea at 3:30 PM.
    • Link: UC Berkeley Astronomy Colloquia
  • SJAA Public Star Party & In-Town Observing
    • When & Where: Friday, Sept 18, 2026, ~7:30–10:30 PM | Houge Park, San Jose, CA
    • Focus: Deep-sky targets (Andromeda, Ring Nebula, Saturn) via visual scopes and live digital EAA smart rigs.
    • Details: Free dark-sky community gathering; red-light discipline strictly observed on the telescope lawn.
    • Link: SJAA Events Calendar

Upcoming Events:
Click to see the next two weeks of events in your browser.


Leave a Reply

Your email address will not be published. Required fields are marked *