Slippers

“Long Island Sound is slipper shell soup.” said my friend as we walked the beach at Milford, Connecticut. Judging from the windrows of shells cast up by the tide; 90% of which were slipper shells, she looked to be spot-on correct.


The world is full of animals (and a few plants) busy earning a living pretending to be something else. A cheetah is a cat pretending to be a dog; a grey fox is a dog pretending to be a cat. Slipper shells are snails pretending to be oysters. They are also girls pretending to be boys, but more on that later.

The Atlantic slipper shell (Crepidula fornicata) is one of the most common shells you can find on any eastern beach in North America, with a few Eastern white slipper shells (Crepidula plana) tossed in just make things confusing. They get their name from the shelf or deck on the inside, which makes them resemble shapeless slippers that have been under the bed for years. The deck extends about a third the length of the shell and serves as an anchor and protection for the internal organs. The Atlantic slipper shell is arched with brown markings with the tip bent downward to one side at the back. It is up to an inch and a half long. The Eastern white slipper shell is white and flattened, sometimes a little convex or concave, and generally a bit smaller. Eastern white slippers seem to prefer the inside of old shells and the underside of old horseshoe crabs.

Eggs are brooded within the female’s shell until they develop into exact miniatures of the adult. Periodically, females lift their shells and push the juveniles out into the cold briny deep. Newly hatched young sink to the bottom, where they scrape algae from hard substrate until they settle down in the shallows. Like oyster larvae or spat, slipper shell babies set on anything hard; rocks, shells, horseshoe crabs, each other.

Once a juvenile sets, it attaches with its muscular foot and remains in the same place forever. It has functionally become an oyster - immobile and filter feeding on the microscopic algae and detritus suspended in the water. Oysters have had gazillions of years practicing filter feeding and have evolved an elegantly simple way of moving large volumes of water past their gills, which rake out food particles and pass them to the gut. It has been said that prior to the European invasion, the entire volume of Chesapeake Bay went through an oyster every three days or so. Slipper shells aren’t quite so efficient. Descended from grazing snails that use a tongue-like organ called a radula to rasp algae off rocks, they have come up with a whole new way of getting food. Mucus is secreted from specialized organs located in the mantle and just in front of the gills; the gills sweep in plankton and other particles that stick to the mucus, and the creature uses its radula to lick the whole thing up and pass it to the stomach. Not a dinner guest who would cause you to break out the good china, but it works well enough to get by.

A slipper shell needs a hard surface on which to live; they live in an environment where this critical resource is scarce and scattered. When a slipper finds a hard surface to colonize, be it a rock, piling, shell, or horseshoe crab, other young slippers are attracted to it. Slippers tend to form piles, with the oldest and biggest on the bottom, the youngest and smallest on the top. Piles can be up to ten shells deep.

Slippers are sequential hermaphrodites. The oldest and biggest is the functional female, the smallest and youngest is the functional male. The animal in between are in various stages of transition from male to female. Female is the fallback gender. When a young slipper colonizes a new surface, it becomes female and releases a pheromone to prevent others from following suite. When the female on the bottom of a stack dies, the next one up becomes female and begins to produce pheromone and eggs.

Hermaphrodism occurs throughout the animal kingdom wherever you get a sedentary species with scattered resources. The familiar orange and white clown fish is just such a species. Clown fish colonize sea anemones. Anemones possess tentacles armed with stinging cells and can capture and devour prey up to and including clown fish size. Clown fish secrete a mucus which the sea anemone chemically recognizes as itself, and which protects the clown fish. Anemones are relatively scattered along the bottom in reef environments, and are the critical resource required by the clown fish. Clown fish form groups living around and defending individual anemones. The biggest and oldest clown fish is the functional female, the next biggest, the male. The rest wait their turn. If the female dies or falls to a predator, the male becomes female and the next biggest clown fish becomes the male. Everybody moves up a notch in the hierarchy. Try explaining the movie Finding Nemo in that context. When little Nemo’s mommy and siblings are eaten by the big bad barracuda, Nemo’s daddy should become Nemo’s new mommy, and little Nemo becomes the new daddy…things go weird from there.

For all that they are mucus-eating, bisexual hermaphroditic snails pretending to be oysters, slipper shells are the most common shell on any beach from Florida to Maine. They must be doing something right.

Starry Messenger

The other night, Alec called from school. He has been pretty much incommunicado this semester, so a phone call was an occasion for some concern. Turns out he was headed back to his dorm after Marching Band practice after dark, when he happened upon the school’s astronomy club. He stopped by to chat, and was shown Comet Holmes. The club members pointed out the location for naked eye viewing and gave him a look through a telescope. He was excited and his first impulse, like ET, was to phone home.

Comet Holmes was discovered in November 1892 by (you guessed it) Mr. Edwin Holmes, a British astronomer. His namesake comet orbits the Sun once every seven years at a distance of about 200 million miles (a little over twice Earth's 93-million-mile orbit). It was re-observed in 1899 and 1906 before being lost for nearly six decades. Based on a prediction from calculations, the comet was found again in 1964.

It is a local (relatively speaking) object, reaching its farthest distance from the sun somewhere between the orbits of Mars and Jupiter. Every seven years it makes the round trip, and has been doing so for who knows how long. What makes this comet remarkable; a once in a lifetime viewing as some authorities have dubbed it, is that it periodically “erupts”. Normally a magnitude 17 object, only visible with a pretty powerful scope, it blossoms to a magnitude 3 object every 100 years or so. Magnitude 3 means it becomes as bright any star and is easily visible to the naked eye. On October 20, in less than 24 hours, it brightened by a factor of nearly 400,000 and has now up to a factor of over a million times what it was before the outburst. This is a change "absolutely unprecedented in the annals of cometary astronomy." The comet is now rivaling some of the brighter stars in the sky. When it first cooked off, some observers thought they were witnessing a super nova – an exploding star. A super nova was last seen in the galactic neighborhood around the time of Keppler and Tycho Brahe.

Theories abound as to why Holmes brightened up ("elementary Watson"--sorry, I couldn't resist), but as yet, no one has come up with anything definitive or remotely plausible. For all we know, Scottie just turned on the warp drive engines. What is amazing is that Holmes made its closest approach to the sun last May and came no closer than 190 million miles to the sun. The comet is now moving away from the sun, boggieing its way back to Jupiter. Not exactly a recipe for the typical show-off Great (notice the initial caps) comet. None the less, there it is, in the constellation Perseus.

You can see Holmes' comet almost any time this fall until it fades, when that will be is anybody's guess since we don't know how it got bright to start with. Some astronomers predict it will grow to rival the full moon in size. Go outside and find the constellation Cassiopeia. That’s the one in the North-east sky that looks like the number “3” as drawn by a first grader. (Tilt you head right and it looks like an “M”, tilt left and it’s a “W”). Find the bottom star in the group and look at about 5 o’clock. You will see a bright star in the Perseus, with a somewhat brighter star about 5 o’clock from it. This star is the top of a triangle. The bottom left star of the triangle is Comet Holmes. Look at it carefully and you will notice it is fuzzy around the edges. Binoculars bring this out even better. I set up my 20x spotting scope on the back deck and even with this relatively puny optics, I was able to see a star shining through the fuzz and the hint of a denser area in the center; the nucleus itself. Way cool.

A well-known astronomer once remarked: “Comets are like cats; they both have tails and they both go where they please.” If that is the case, then Comet 17P/Holmes must be of the Manx variety. Unlike some the so-called Great Comets (Haley on most occasions in the past thousand years, or Halle-Bop from a few years ago), Holmes does not possess a tail to speak of. Most comets can be described as “dirty snowballs,” consisting mostly of ice with chunks of rock embedded in. It may be that Holmes, with its seven-year run, has had most of the ice already ablated off the nucleus and is pretty much solid rock…or not. Like cats, comets are pretty much inscrutable.