NASA's #ParkerSolarProbe was able to image the surface of #Venus from space in a way we didn't think possible before!
Here, we can see the Aphrodite Terra highland *glowing* through the clouds (left), exactly where radar data tell us it should be (right)!
Venus' thick cloud layer obscures the surface from space at visible wavelengths—but there are some "windows" at near-infrared wavelengths where cameras can see through to the surface.
PSP took these images at a wavelength not thought to be able to penetrate the clouds before.
This matters because, unlike Mars, Mercury, the Moon, etc, we can't easily see the Venus surface—we have to use radar.
But if we can "see" the surface in the near infrared, we can start to learn things about what it's made of. And thus we can learn new things about Venus.
The new VERITAS and EnVision missions will have similar camera systems, which will use multiple NIR wavelengths to see the surface.
The atmosphere "scatters" light, so these images will be very low resolution.
But at a global scale, they'll be *invaluable*.
And, besides, Parker Solar Probe is a mission to investigate the *Sun*, so getting *photos of the surface of Venus* OPPORTUNISTICALLY is just another example of how amazing—and fortuitous—spacecraft exploration can be!
A quick 🧵 about the *size* of the #HungaTonga eruption:
Volcanic eruptions are generally assigned a VEI—Volcanic Explosivity Index—value.
This scale is a general indicator of the explosive character of an eruptive event.
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This scale, described by Christopher Newhall and Stephen Self in a 1982 paper, is a general indicator of the explosive character of an eruptive event, and reflects the interplay of an eruption's magnitude, intensity, and energy release rate.
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The VEI rating scale employs a set of criteria including ejecta volume, style of eruption, plume height, and injection of gases into the troposphere and stratosphere.
There's no question that the #Tongaeruption was huge—it absolutely was.
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I need you to know I'm being completely serious here.
We have no idea what's inside Uranus.
We really don't have a clue what's inside this or there other "ice giant", Neptune.
It's possible that there's a rocky interior, perhaps at least as large as Earth. There might be a water–ammonia ocean above that rocky centre, topped with a thick atmosphere.
But we don't know.
Uranus and Neptune are the outer Solar System's Venus -- fascinating, largely unexplained, but to be honest pretty much ignored in the modern era of planetary exploration.
The Solar System is *full* of incredible and fascinating worlds!
Mercury.
Venus.
Earth.
The Moon.
Jupiter.
Saturn.
Uranus and Neptune.
Ceres, Vesta, and the other main asteroid belt bodies.
The myriad other minor bodies scattered across the System.
Every one of them amazing! 🥰
People are pointing out that I forgot somewhere important!
Somewhere that fascinates everyone, that we need to explore more, that holds a special place in our heart.
Interested in learning more about #Venus—and why @NASA's decision to go back there with the #VERITAS and #DAVINCI+ missions is such a big flippin' deal?
Venus and Earth are the same(ish) size, age, and composition (in roughly the ~same proportions), orbiting the same star.
So, uh... what's going on?
Here's where we come to our two different stories for Venus—and why figuring out which one is correct is *critical* to understanding not only our own world, but Earth-size worlds everywhere.