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Uranus Lights Up for Hubble

HST images of Uranus’ aurorae and rings combined with Voyager 2 images of the planet itself. (NASA)

Those white areas aren’t clouds; they’re aurorae—”northern lights”—around the poles of Uranus, captured by the Hubble Space Telescope in 2012 and 2014. (The image of Uranus itself was acquired by the Voyager 2 spacecraft in January 1986.)

“The auroras on Jupiter and Saturn are well-studied, but not much is known about the auroras of the giant ice planet Uranus. In 2011, the NASA/ESA Hubble Space Telescope became the first Earth-based telescope to snap an image of the auroras on Uranus. In 2012 and 2014 a team led by an astronomer from Paris Observatory took a second look at the auroras using the ultraviolet capabilities of the Space Telescope Imaging Spectrograph (STIS) installed on Hubble.”

Aurorae on Uranus are driven by the same process that creates them around Earth’s polar regions: charged particles from the Sun get caught in the planet’s magnetic field and are focused toward the poles, where they make ions in the upper atmosphere release energy—in these observations in ultraviolet wavelengths. Also, since Uranus orbits the Sun “tilted sideways” its polar regions are near the plane of its orbit.

Read the rest of this article from NASA here: Hubble Spots Auroras on Uranus


Here’s Hubble’s Newest Knockout Portrait of Jupiter

Jupiter imaged by the Hubble Space Telescope on April 3, 2017. Credit: NASA, ESA, and A. Simon (GSFC)

On April 3, 2017, as Jupiter made its nearest approach to Earth in a year, NASA’s Hubble Space Telescope viewed the solar system’s largest planet in all of its up-close glory. At a distance of 415 million miles (668 million km) from Earth, Jupiter offered spectacular views of its colorful, roiling atmosphere, the legendary Great Red Spot, and its smaller companion at farther southern latitudes dubbed “Red Spot Jr.” Taken with Hubble’s Wide Field Camera 3, the image resolves details in Jupiter’s atmosphere as small as about 80 miles (129 km) across.

Read the full article on NASA’s Hubble site here, and check out a version I made with enhanced contrast and sharpness to bring out some details in Jupiter’s clouds below:

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This Blazing Quasar Got Wave Motion Gunned Clear Out Of Its Galaxy

Hubble image of quasar 3C 186 racing out of from its host galaxy, 8 billion light-years away from Earth. Credit: NASA, ESA, and M. Chiaberge (STScI and JHU).

Astronomers still have yet to directly capture an image of a black hole—they’re working on it—but they know where some of the largest ones are: inside the hearts of galaxies, where they power brilliant and powerful quasars whose light can be seen across the Universe. Some of these supermassive black holes (SMBs) can contain the mass of millions if not billions of Sun-sized stars and, when two galaxies happen to collide (which they often do) their respective resident SMBs can end up locked in an orbital embrace. As their spinning dance grows tighter and tighter they send out gravitational waves, rippling the very fabric of space and time itself (the LIGO experiment announced the first detection of these waves in 2016.) But if the gravitational waves are uneven, say because the two merging SMBs are of vastly different masses and/or individually spinning in different orientations (a possible but not common scenario) then the super-duper-supermassive black hole that results from the merger can end up getting one serious cosmic-scale kick after the event occurs and the waves shut off—perhaps a strong enough kick to send it hurtling out of the galaxy altogether.

That’s what astronomers think we’re witnessing here in this image from the Hubble Space Telescope.

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No, the Solar System (Still) Isn’t a Vortex

Animation of a “vortex” Solar System. (Credit: DjSadhu)

Like a bad penny (or a grossly inaccurate science meme) this tends to rear its shiny animated head online at least a couple of times a year, and it seems this year will be no exception. It’s a GIF showing the motions of the Sun and planets through space, trailing glowing lines (which they don’t but that’s just an illustration) in order to “prove” that the Solar System is really a vortex and vortices are cosmically significant and life is magic and ehrmagerd your mind should = blown. Or something like that.

Except, other than being a pretty animation, it’s simply not the case. The creator, DjSadhu, is much more metaphysicist than astrophysicist (really he’s a music and video producer) and ultimately what he was supporting is a reconstruction of the heliocentric model and an alternate path of the Sun around the galaxy itself, which is simply just wrong. Luckily an astrophysicist and an astronomer—Rhys Taylor and Phil Plait, respectively—were more than willing to offer their professional opinions on the matter when this all first appeared, the former writing a blog post in response to the latter’s. I was able to convince Rhys to let me share his post on Universe Today, and it offers a lot of entertaining insight as to why that little animation is not only misleading but the herald of a slew of inaccuracies.

Read the full debunking on Universe Today: Is the Solar System Really a Vortex?

Note: A year after the original article(s) were published Rhys shared another in which he commends Sadhu for openly communicating about the physics involved and actually creating a more accurate version of the animation—and without the unscientific woo. You can (and I suggest you do) read that post here. Unfortunately on the internet nothing ever really goes away, so the first GIF inevitably shows up every now and then. Remember all this the next time it does.

NOAA and NASA Open a New Set of Eyes on the Sun

These images of the sun were captured at the same time on January 29, 2017 by the six channels on the SUVI instrument on board GOES-16 (Credit: NOAA)

These images of the sun were captured on January 29, 2017 by the six channels on the SUVI instrument on board GOES-16. (Credit: NOAA)

Look out SDO—there’s another set of eyes watching the Sun in a wide swath of wavelengths! The images above are the first from the Solar Ultraviolet Imager (SUVI) instrument aboard NOAA’s new GOES-16 satellite, positioned in a geostationary orbit about 22,200 miles from Earth. These are SUVI’s first successful test images, captured on Jan. 29, 2017; once fully operational SUVI will monitor the Sun round the clock in six different UV and X-ray wavelengths, providing up-to-date data on the behavior of our home star.

Watch the first video of the Sun from GOES-16 data below:

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