Learn

Small ideas, carefully kept.

8 short entries, about 2 minutes in all. Each stands on its own, with its sources beside it. Open what interests you; save what you want to keep.

Loading your progress…

  1. Half the people counting passes never saw the gorilla.

    In a classic experiment, about half the viewers who were busy counting basketball passes failed to notice a person in a gorilla suit walk through the scene 1. Attention does not just highlight what matters; it quietly deletes the rest.

    Try it

    Next time you search for your keys, notice how many objects on the table you could not name a moment later.

    Go deeper1 min

    The result is called inattentional blindness: failing to see something fully visible because attention is engaged elsewhere. It is not a failure of the eyes. The light from the gorilla reached every viewer's retina.

    Two details in the study make it more interesting than a party trick 1:

    • Harder tasks deleted more. Viewers keeping separate counts of bounce passes and aerial passes noticed the gorilla less often than those keeping a single count.
    • Similarity mattered. Viewers tracking the team in black noticed the black gorilla more often than those tracking the team in white.

    So attention behaves less like a spotlight that adds light and more like a filter tuned to a goal. Whatever does not match the goal is treated as noise, even when it is a gorilla.

    Read the essay: The Quiet Work of Attention
  2. Memory doesn’t fade in a straight line. It drops fast, then levels out.

    When Hermann Ebbinghaus memorised lists of nonsense syllables and measured how much effort relearning saved, most of the loss came within the first day; after that, forgetting slowed to a crawl 1.

    A line chart of memory savings falling steeply in the first day and flattening over a month. 60%40%20%0% 20m1h9h1d2d6d31d Time since learning (log scale) 58%44%21%
    Ebbinghaus’s own measurements, 1885. “Savings” is how much less time relearning took 1.
    Read the diagram as text

    Savings in relearning, by time since learning. 20 minutes, about 58 percent. 1 hour, about 44 percent. 9 hours, about 36 percent. 1 day, about 34 percent. 2 days, about 28 percent. 6 days, about 25 percent. 31 days, about 21 percent.

    Go deeper1 min

    Ebbinghaus was his own and only subject, which is a reason for caution. But the shape of his curve has been found again and again: steep at first, then shallow.

    The practical consequence is spacing. Reviewing just as something begins to slip, and then waiting longer before the next review, makes each review count for more. A large review of the research found that spreading practice out beats cramming it together, and that the best gap grows with how long you want to remember 2.

    A reasonable starting rhythm: revisit something the next day, then after a few days, then after a couple of weeks.

    Read the essay: Curiosity Is a Practice, Not a Mood
  3. Rereading feels like learning. Testing yourself actually is.

    Students who read a passage once and then practised recalling it remembered much more a week later than students who spent the same time rereading it, even though rereading looked better on a test five minutes later 1.

    Try it

    Close this page and say the main idea of this entry out loud. That small effort is the effect at work.

    Go deeper1 min

    In the study, one group read a short passage four times. Another read it once and then tried to write down everything they could recall, three times over 1.

    Five minutes later, the rereaders did better. A week later the result reversed: the group that practised recall remembered about 61 percent of the ideas, the rereaders about 40 percent. The rereaders were also more confident they would remember.

    That gap between how learning feels and how well it lasts is the useful part. Fluency, the smooth sense of “I know this”, comes cheaply from rereading. Retrieval is effortful, and the effort is what strengthens the memory.

    Read the essay: On Reading Slowly
  4. Your brain is about 2% of your body and uses about 20% of its energy.

    An adult brain weighs roughly 2 percent of the body yet accounts for about a fifth of its resting energy use, and most of that goes into ongoing activity rather than into any particular task 1.

    Go deeper1 min

    The surprising part is not the size of the budget but how little of it changes. When you start a demanding task, the extra energy the brain uses in the regions involved is small compared with what it was already spending 1.

    In other words, the brain is never idle. Much of its cost is the constant work of keeping neurons ready to signal and of activity that goes on whether or not you are concentrating. A hard problem adds a little on top; it does not switch the engine on.

    Read the essay: What a Single Neuron Can Compute
  5. A single human neuron can solve a problem once thought to need a network.

    Recordings from human cortical neurons found a kind of electrical spike in the dendrites that is strongest for moderate input and weaker for strong input, which lets one cell compute “exclusive or”, a function textbooks said needed two layers of neurons 1.

    Go deeper1 min

    Exclusive or (XOR) answers “yes” when exactly one of two inputs is on:

    • neither input: no
    • input A only: yes
    • input B only: yes
    • both inputs: no

    A simple model neuron adds its inputs and fires above a threshold, so “both” always looks like more than “one”. It cannot say no to both. That limit is why XOR became the standard example of what single units cannot do.

    The dendritic spikes in the study behaved differently: they were largest near threshold and shrank as input grew stronger 1. A response that falls off with too much input is exactly what XOR needs. The finding does not make a neuron a computer, but it suggests a single cell is closer to a small network than to a single switch.

    Read the essay: What a Single Neuron Can Compute
  6. Entropy isn’t really “disorder”. It’s a count of ways.

    Ludwig Boltzmann defined entropy by counting how many microscopic arrangements look the same from the outside 1. Mixed states win not because nature prefers mess, but because there are vastly more ways to be mixed.

    A bar chart of the number of ways four coins can show zero to four heads: 1, 4, 6, 4, 1. 14641 0 heads1 head2 heads3 heads4 heads Ways four coins can land (16 in all)
    Four coins. The half-and-half outcome can happen six ways; all heads only one.
    Read the diagram as text

    Four coins, sixteen possible arrangements. Zero heads, 1 way. One head, 4 ways. Two heads, 6 ways. Three heads, 4 ways. Four heads, 1 way. The evenly mixed outcome, two heads, has the most arrangements, so it has the highest entropy.

    Go deeper1 min

    Boltzmann’s formula, carved on his tombstone, is S = k log W: entropy S grows with the number of arrangements W 1.

    With four coins the difference is modest: six ways to be half and half, one way to be all heads. With the trillions of trillions of molecules in a cup of coffee, the mixed states outnumber the tidy ones by margins so large that “unlikely” becomes “never seen”.

    That is also why entropy is tied to the direction of time. A system wandering among its possible arrangements will almost certainly drift toward the overwhelming majority. The puzzle, as Carroll argues at length, is not why entropy rises but why it started so low 2.

    Read the essay: Why Time Seems to Have a Direction
  7. The sunlight on your skin left the Sun about 8 minutes and 19 seconds ago.

    The astronomical unit, the average Earth–Sun distance, is defined as exactly 149,597,870,700 metres 1. Divide by the speed of light, exactly 299,792,458 metres per second 2, and you get about 499 seconds.

    Try it

    Look at a patch of sunlight and count to 499. That is how long it was on its way.

    Go deeper1 min

    The distance changes through the year, because Earth’s orbit is slightly elliptical, so the travel time runs from roughly 8 minutes 10 seconds in early January to about 8 minutes 27 seconds in early July.

    The light’s journey across space is the short part. The energy it carries was released by fusion in the Sun’s core, and reaching the surface takes far longer, because radiation is absorbed and re-emitted countless times on the way out. One estimate puts that at around 170,000 years 3.

    Read the essay: Why Time Seems to Have a Direction
  8. “You must not fool yourself — and you are the easiest person to fool.”

    Richard Feynman’s 1974 Caltech commencement talk argued that scientific integrity means reporting everything that could make your result wrong, not only what supports it 1.

    The first principle is that you must not fool yourself—and you are the easiest person to fool.

    Richard Feynman, Cargo Cult Science, 1974 1
    Go deeper1 min

    Feynman’s examples were experiments that copied the outward form of science without its substance: the right rituals, but no honest test that could have proven them wrong.

    The practical version is a habit of asking, before you share a conclusion: what would I expect to see if I were wrong, and did I look for it? The talk calls this “leaning over backwards” 1. It is uncomfortable precisely because the person most motivated to miss the flaw is you.

    Read the essay: Curiosity Is a Practice, Not a Mood

End of this set

That’s everything, for now.

You’ve reached the last of 8 entries. Nothing loads below this line, by design.

What you kept

Nothing saved yet. Use Save on any entry to keep it in this browser.

A full essay

The Quiet Work of Attention

2 min read

Back to the first entry

Saved in this browser

Saved entries stay on this device only. No account, nothing uploaded.

Nothing saved yet. Use Save on an entry to keep it here.

Download a copy

Creates a Markdown file (.md) of your saved entries and their sources. Separate from saving: the file is yours to keep anywhere.