• =?UTF-8?Q?Is_Earth_an_Oddball=3F_One_of_the_Strangest_Things_in_the?= =

    From a425couple@21:1/5 to All on Sun Dec 15 12:54:59 2024
    XPost: alt.astronomy, alt.fan.heinlein

    In the old days, especially in Sci-Fi, it was felt once we could
    explore, we would find plenty of places to live, just like Earth.

    from https://scitechdaily.com/is-earth-an-oddball-one-of-the-strangest-things-in-the-cosmos-might-be-us/

    Is Earth an Oddball? One of the Strangest Things in the Cosmos Might Be – Us By Pat Brennan, NASA's Exoplanet Exploration ProgramJanuary 1, 202229
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    Earth Rotating Sun Space
    How rare in the galaxy are rocky planets like Earth in similar orbits
    around Sun-like stars? The question turns out to be surprisingly
    difficult to answer.
    Despite thousands of exoplanets discovered, Earth remains unique in its
    size, orbit, and type of star. Technical challenges in current detection methods make finding Earth-like planets difficult, especially around
    Sun-like stars, leading to uncertainties about whether our solar
    system’s arrangement is rare or just hard to detect.

    One of the strangest things in the cosmos might be – us.

    Among the thousands of planets confirmed to be in orbit around other
    stars, we’ve found nothing quite like our home planet. Other planets in Earth’s size range? Sure, by the bushel. But also orbiting a star like
    our Sun, at a comparable distance? So far it’s just one, lonely example.
    The one beneath our feet.

    A big part of this is likely to be the technical difficulty of finding a
    sister planet. Our telescopes, in space and on the ground, find planets
    around other stars by two main methods: wobbles and shadows.

    The “wobble” method, or radial velocity, traces the subtle
    back-and-forth motion as orbiting planets tug their star this way, then
    that, because of gravity. The larger the tug, the “heavier” the planet — that is, the greater its mass.

    In the search for shadows, planet-hunting telescopes wait for a tiny dip
    in starlight as a planet crosses the face of its star — a crossing known
    as a “transit.” The bigger the dip, the wider the planet.

    In both cases, large planets are much easier to detect than small ones.
    And in the case of transits, small, rocky planets about the size of
    Earth show up much better against very small stars known as red dwarfs.
    In a sense, they cast a bigger shadow that blots out proportionally more
    of a small star’s light, so instruments like NASA’s TESS space telescope can more readily find them. A Sun-sized star won’t dim as much when an Earth-size planet passes by, making their transits harder to detect.

    Apollo 11 Earth Image
    Apollo 11 Earth image. Credit: NASA Johnson Space Center
    And there’s another troubling issue: time. A planet orbiting a star at Earth’s distance from the Sun would take about 365 days to make one revolution – just like our planet’s “year.” But to confirm such an orbit, your telescope would have to stare at that star for, say, 365
    days to catch even one transit — and to be sure it’s truly a planet, you’ll want to see at least two or three of these transit signals.

    All of these difficulties have placed such planets largely out of reach
    for today’s instruments. We’ve found plenty of small, rocky planets, but they’re nearly all orbiting red dwarf stars.

    In our galaxy, red dwarfs are far more common than larger yellow stars
    like our Sun. That still leaves room for billions of Sun-like stars and,
    maybe, a significant number of habitable, Earth-sized worlds circling them.

    Or maybe not.

    Rare or Just Difficult?
    The apparent oddness of our home system doesn’t end with Earth. Our particular arrangement – small, rocky worlds in the nearest orbits, big
    gas giants farther out – also is something we haven’t yet detected in
    close parallel anywhere else. Whether this is because they are truly
    scarce or because they are hard to detect is unclear.

    Jupiter takes one trip around the Sun every 12 years. But Jupiter-type
    planets in long orbits are comparatively rare around other stars, and
    that could be important. Theorists say Jupiter might well have cleared
    the way for Earth to become a habitable world, quite literally. The
    giant planet’s intense gravity could have hoovered up small rocky bits
    that might otherwise have smashed into Earth, sterilizing it just as
    life was getting its start.

    “The planetary systems we are finding do not look like our solar
    system,” said Jessie Christiansen, a research scientist at NASA’s
    Exoplanet Science Institute. “Is it important that our solar system is different? We don’t know yet.”

    Christiansen, who studies exoplanet demographics, does not think
    “Earths” will turn out to be rare, but says scientific literature on the question “is all over the place.”

    Far more data are needed, scientists tell us, to determine the frequency
    of planets similar to Earth in both size and circumstance.

    Future space telescopes could examine the atmospheres of distant, rocky
    worlds for signs of oxygen, methane, or carbon dioxide – in other words,
    an atmosphere that reminds us of home.

    For now, we remain in the dark. Earth-like planets around Sun-like stars
    might be plentiful. Or, they could be the true oddballs of the galaxy.

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