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Opportunity Spots Phobos Skimming the Sun

Animation of raw panorama camera images from NASA’s Opportunity rover on May 3, 2017. NASA/JPL-Caltech; animation by Jason Major

It may be in its 14th year on Mars but Opportunity still has some surprises to show us—like this, a series of images captured on May 3, 2017 showing the Sun as seen from Mars. But that’s not the special part: see the change in brightness along the Sun’s edge near the end? That was a brief transit of Phobos, the largest (and nearest) of Mars’ two moons!

Can’t see it very well? It’s quick, I know—so check out a cropped and enlarged version below:

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A Departing View From Cassini After Clearing the Gap

Animation of raw uncalibrated images acquired by Cassini on May 3, 2017 (Credits: NASA/JPL-Caltech/SSI. Animation by Jason Major.)

Cassini did it again! On May 2-3, 2017 the spacecraft made its second “ring dive” pass of Saturn, passing through the clear space between the innermost edge of the ring system and the planet itself. The animation above shows a view from Cassini looking back toward Saturn on its outbound flight on May 3, just a few hours after the ringplane crossing. Saturn’s limb is visible at upper left.

What’s more, NASA has released a detailed video from the first ring dive on April 26, showing all of the images that were captured and where on Saturn Cassini’s cameras were pointed. Check it out below.

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The Color Out Of Space: What’s False and What’s Real (and Why It’s a Big Deal)

Color-composite of Saturn made from raw, uncalibrated images acquired on May 1, 2004. Warning: NOT SCIENTIFICALLY ACCURATE COLOR.

As you must certainly know by now, I love pictures of the many worlds of our Solar System. That is what I built this blog around and it’s what I’ve been mainly sharing here for the past eight years and counting. I particularly love the pictures of Saturn from NASA’s Cassini mission…really nothing exemplifies the beauty of the Solar System for me like majestic sweeping views of Saturn’s rings. And thanks to the modern marvel of The Internet these images have been made available to everyone, nearly as the same time as they are to the scientists on the mission team. This is true for many of NASA’s recent and current missions, not just Cassini, and there is a constantly-growing group of enthusiasts out there who take these raw images and create beautiful, full-color pictures from them, helping to bring the wonders of the Solar System to life.

There is a downside to doing this. The color images that are being produced by amateurs (including myself) are not usually calibrated to any specific standards. They are composed from preliminary, uncatalogued raw images. These usually—but not always—have been acquired in visible-light wavelengths, but even then the result isn’t necessarily an accurate representation of the colors you’d see if you were looking at the same scene from the viewpoint of the spacecraft.

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Cassini Survived Its Historic First Pass Between Saturn and Rings; First Pics In!

An image of Saturn’s north polar vortex captured by Cassini on April 26, 2017. (NASA/JPL-Caltech/SSI)

Cassini made it! On April 26, 2017, NASA’s Saturn-exploring spacecraft made its closest pass by the planet since its arrival in 2004, beginning the final phase of its mission with its first “Grand Finale” orbital pass that took it between the top of the planet’s atmosphere and the innermost edge of the ring system. It’s literally a journey that no other spacecraft has ever made—and now the pictures are coming in!

It’s also the closest Cassini has come to Saturn itself; at closest point Cassini was only about 1,900 miles (3,000 km) above the tops of Saturn’s swirling clouds. It’s amazing to think that the images we’re seeing were captured with Cassini’s wide angle camera—typically views like this have had to use its “zoom” narrow-angle camera!

Check out an animation below of some of Cassini’s views captured during the pass over Saturn’s north pole.

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Cute Science Video Alert: The Story of Stars

Like people, stars are found in all colors and sizes. They can range from small, sassy red dwarfs to giant blue beasts. In fact there are seven main types of stars, grouped by their apparent colors (and thus temperatures) and classified as O, B, A, F, G, K, or M in order of hottest to coolest. (Learn more about that here.) The video above, released by The Royal Observatory in Greenwich, England, gives a brief life history of three of the most common types of stars found in our galaxy: blue O stars, red M dwarfs, and yellow G stars—the latter of which being the class of our own Sun. It’s really fun, cute, and educational—check it out, and also find more videos on The Royal Observatory’s Vimeo page. 

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