Category: Space

  • Why Do Stars Twinkle?

    The star itself is not rapidly brightening and dimming.

    The twinkle is being added much closer to home.

    Earth’s atmosphere is constantly moving.

    Starlight passes through changing air

    Different pockets of air have slightly different temperatures and densities.

    As starlight travels through those layers, the light bends by tiny changing amounts.

    The path is never perfectly steady.

    That changing refraction makes the star seem to shift, brighten, or dim from moment to moment.

    Why are stars especially affected?

    Stars are so far away that they look like tiny points of light.

    Because the apparent source is so small, little changes in the light path can noticeably affect what reaches your eye.

    Why do planets usually twinkle less?

    A planet may look like a point to your naked eye, but it actually presents a tiny disk.

    Light reaches you from several parts of that disk at once.

    Atmospheric distortions affecting one part can average against distortions affecting another.

    That usually makes planets appear steadier than stars.

    Do stars twinkle in space?

    Not for the same reason.

    Astronauts above Earth’s atmosphere do not have the same moving layers of air between them and the stars.

    Remove the atmosphere and you remove the main source of ordinary twinkling.

    Is this related to mirages?

    Both involve light bending through air with different temperatures and densities.

    A hot-road mirage is a much stronger everyday example of atmospheric refraction near the ground.

    Star twinkling comes from smaller, constantly changing distortions spread through the atmosphere.

    Why do stars near the horizon often twinkle more?

    Their light has to travel through more atmosphere before reaching you.

    More air means more opportunities for the light path to be disturbed.

    So the star is not flickering like a distant light bulb.

    Earth’s moving atmosphere is adding the twinkle.

    And that’s the short explanation.

    Related explanations: Why does a hot road look wet?, Why does a straw look bent in water?, and Why do airplanes leave white trails?

  • Why Do We Have Day and Night? Earth Is Turning You Toward and Away From the Sun

    We have day and night because Earth rotates on its axis.

    At any moment, roughly half of Earth faces the Sun and receives sunlight. The other half faces away and is in darkness.

    As the planet turns, your location moves from the dark side into sunlight and then back into darkness.

    One spin produces the basic daily cycle.

    Earth rotates from west to east

    Earth turns eastward.

    Because we are riding on the rotating planet, the Sun appears to move in the opposite direction across the sky, rising in the east and setting in the west.

    The Sun is not actually circling Earth once every day.

    The apparent motion mostly comes from us rotating underneath it.

    One day is about one rotation

    Relative to the Sun, Earth’s rotation gives us a solar day of about 24 hours.

    Relative to distant stars, Earth completes a rotation in slightly less time, about 23 hours and 56 minutes.

    The difference exists because Earth is also moving along its orbit around the Sun. It has to rotate a little farther each day before the Sun returns to the same apparent position in the sky.

    For ordinary life and clocks, 24 hours is the useful number.

    Why is it daytime in one country and nighttime in another?

    Because Earth is round.

    While one side faces the Sun, places on the opposite side face away.

    When it is noon in one region, another region may be near midnight.

    Time zones are our human system for organizing that rotating geometry into clocks.

    The planet does not know what time zone it is in.

    It just keeps turning.

    Why are days longer in summer?

    Earth’s axial tilt affects how long a particular location spends in sunlight during different parts of the year.

    When your hemisphere tilts toward the Sun, your path through the sunlit half of Earth is longer. That produces longer days.

    When your hemisphere tilts away, the daylight portion is shorter.

    So rotation creates day and night, while Earth’s tilt changes how long each lasts through the seasons.

    What is the line between day and night called?

    The boundary between the illuminated and dark halves of a planet is called the terminator.

    From space, it appears as a broad dividing region rather than a razor-thin line because Earth’s atmosphere scatters sunlight and creates twilight.

    As Earth rotates, locations cross that boundary at sunrise and sunset.

    If Earth is spinning so fast, why do we not feel it?

    At the equator, Earth’s surface moves at roughly 1,000 miles per hour due to rotation.

    You do not feel steady motion very well when you, the ground, the atmosphere, and almost everything around you are moving together.

    You mainly feel changes in motion, such as acceleration, braking, or turning sharply.

    Earth’s rotation is smooth enough that daily life does not feel like a carnival ride.

    Thankfully.

    So sunrise and sunset are not the Sun switching on and off.

    They are what it looks like from a planet that refuses to stop spinning.

    A related part of the natural world appears in Why Does Earth Have Seasons?, where the same kind of physical or biological reasoning answers another familiar question.

    And that’s the short explanation.

    Related explanations: Why Does Earth Have Seasons? and Why Does the Moon Have Phases?

  • Why Does the Moon Have Phases? The Moon Is Not Changing Shape

    The Moon has phases because it orbits Earth while sunlight illuminates half of it.

    The Moon itself is not growing, shrinking, or changing shape. What changes is how much of its sunlit half we can see from Earth.

    That shifting geometry produces the familiar new moon, crescent, quarter, gibbous, and full moon phases.

    Half the Moon is almost always lit by the Sun

    Just as Earth has a day side and a night side, the Moon has a sunlit side and a dark side.

    At nearly any moment, one half of the Moon is illuminated by the Sun.

    The important question is how that lit half is oriented relative to us.

    As the Moon travels around Earth, our viewing angle changes.

    New moon happens when the lit side faces mostly away from us

    During a new moon, the Moon is located roughly between Earth and the Sun.

    The half facing the Sun is bright, but most of that illuminated side faces away from Earth.

    From our viewpoint, the Moon appears dark or nearly invisible.

    The Moon did not stop reflecting sunlight.

    We are simply looking mostly at the night side.

    A full moon is the opposite geometry

    About two weeks later, Earth is roughly between the Sun and Moon.

    Now the Moon’s sunlit half faces toward us, and we see an almost fully illuminated disk.

    That is the full moon.

    Between those two positions, we see different fractions of the lit half.

    What are crescent, quarter, and gibbous phases?

    A crescent moon shows less than half of the visible disk illuminated.

    At first quarter and third quarter, we see half of the Moon’s visible face illuminated. The name “quarter” refers to the Moon being about one-quarter or three-quarters of the way through its orbit, not to seeing one quarter of the Moon.

    A gibbous moon shows more than half but less than the full disk.

    When the illuminated portion is increasing, the Moon is waxing. When it is decreasing, the Moon is waning.

    Does Earth’s shadow cause the phases?

    No.

    Earth’s shadow causes a lunar eclipse, which is a different event.

    If Earth’s shadow created the ordinary phases, lunar eclipses would happen every month and the geometry would look very different.

    Moon phases are produced simply by our changing view of the Moon’s sunlit half.

    This distinction is one of the biggest misconceptions about the Moon.

    How long does the phase cycle take?

    From one new moon to the next takes about 29.5 days.

    During that time, the Moon completes the familiar sequence of phases.

    That is why the lunar cycle and the idea of a month have been connected in human calendars for thousands of years.

    Why do we always see roughly the same side of the Moon?

    The Moon rotates once on its axis in about the same amount of time it takes to orbit Earth.

    That synchronized rotation keeps nearly the same hemisphere facing us.

    It does not mean the Moon does not rotate.

    In fact, if it did not rotate at all, we would eventually see every side as it traveled around Earth.

    So the changing Moon in the night sky is not a shape-changing object and not a monthly shadow show.

    It is geometry.

    Sunlight illuminates half.

    The Moon moves.

    Our viewpoint changes.

    And the sky gives us a different-looking Moon almost every night.

    A related part of the natural world appears in Why Does Earth Have Seasons?, where the same kind of physical or biological reasoning answers another familiar question.

    And that’s the short explanation.

    Related explanations: Why Does Earth Have Seasons? and Why Do We Have Day and Night?

  • Why Does Earth Have Seasons? It Is the Tilt, Not the Distance From the Sun

    Earth has seasons because its axis is tilted.

    The planet does not spin straight up and down relative to the plane of its orbit around the Sun. Its axis is tilted about 23.4 degrees.

    As Earth travels around the Sun during the year, that tilt changes how directly sunlight strikes each hemisphere and how many hours of daylight it receives.

    Earth’s distance from the Sun is not the main reason

    This is one of the most common misconceptions about seasons.

    It feels logical that summer should happen when Earth is closer to the Sun and winter when it is farther away.

    But the timing does not work.

    Earth is actually closest to the Sun in early January, during winter in the Northern Hemisphere. It is farther away in early July, during northern summer.

    The small change in orbital distance is not what creates the familiar seasonal cycle.

    Tilt changes the angle of sunlight

    Imagine shining a flashlight straight down onto a table. The light is concentrated in a relatively small area.

    Now tilt the flashlight. The same amount of light spreads over a larger area.

    Sunlight works similarly.

    When a hemisphere is tilted toward the Sun, sunlight strikes it more directly. Solar energy is more concentrated, which contributes to warmer temperatures.

    When the hemisphere tilts away, sunlight arrives at a lower angle and spreads over a larger area.

    Tilt also changes day length

    Summer is not just about the angle of the Sun.

    When your hemisphere is tilted toward the Sun, the Sun stays above the horizon longer each day. Longer daylight gives the ground and atmosphere more time to absorb solar energy.

    In winter, days are shorter and the Sun stays lower in the sky.

    Less direct sunlight plus fewer daylight hours creates a powerful seasonal difference.

    Why are the seasons opposite in the two hemispheres?

    When the Northern Hemisphere tilts toward the Sun, the Southern Hemisphere tilts away.

    That is why June can mean summer in the United States and winter in Australia.

    Six months later, the geometry reverses.

    If distance from the Sun caused the seasons, both hemispheres would have summer at the same time.

    They do not.

    That is another easy way to test the idea.

    What happens during spring and fall?

    Around the equinoxes, neither hemisphere is tilted strongly toward or away from the Sun.

    Day and night are close to equal in length across much of Earth, and the angle of sunlight falls between the summer and winter extremes.

    The seasons then continue shifting as Earth moves along its orbit.

    Why are seasons weaker near the equator?

    Near the equator, day length and the angle of sunlight change less dramatically through the year.

    Higher latitudes experience much larger changes, including very long summer days and very short winter days.

    That is why the difference between seasons is generally stronger as you move farther from the equator.

    Does Earth’s tilt ever change?

    Yes, slowly.

    Earth’s axial tilt varies over very long time periods. Those changes can influence climate patterns over tens of thousands of years.

    But for the everyday yearly seasons you experience, the explanation is straightforward.

    Earth is tilted.

    It goes around the Sun.

    The tilt keeps pointing in nearly the same direction as the planet travels.

    That is enough to turn one orbit into spring, summer, fall, and winter.

    A related part of the natural world appears in Why Does the Moon Have Phases?, where the same kind of physical or biological reasoning answers another familiar question.

    And that’s the short explanation.

    Related explanations: Why Does the Moon Have Phases? and Why Do We Have Day and Night?