2017年2月21日 星期二

Did Voyager 1 capture an image of Enceladus' plumes erupting?


Did Voyager 1 capture an image of Enceladus' plumes erupting?

Posted by Ted Stryk

21-02-2017 13:38 CST

Topics: Enceladus, pretty pictures, amateur image processing, Voyager 1 and 2, Saturn's moons, many worlds, Saturn, explaining image processing

From the moment I first found out about the discovery of geysers erupting into space by NASA's Cassini mission, I began to wonder whether they had been detected before. Pioneer data is of insufficient quality to detect them, but Voyager definitely could have. I carefully examined all of the images targeting Enceladus, but the illumination angle wasn't ideal (very high phase, or backlit, images are best for this, but none of the available images were taken at such an angle). I came up empty handed and dropped project.

Flash forward to the New Horizons Pluto encounter in the summer of 2015. I was sitting in a plenary meeting and the high phase images of Pluto's atmosphere were being discussed for the first time. Later in the meeting, someone asked a question about serendipitous images that might contain Pluto's small moons. The next talk was particle and fields stuff that I didn't really understand, so my mind wandered, and it clicked - maybe Enceladus made a serendipitous appearance in some high phase Saturn images.

In the fall of 2016, I finally found time to work on this. While Voyager 2 had the better camera, due to a spacecraft anomaly, it was not taking pictures during the first few days after closest approach, so after a check to see if there was anything from right after it was recovered, I moved on to Voyager 1. I experimented with some imagery from a few days out to get familiar with its cameras under these conditions before beginning in earnest. This image of Saturn came from this effort.

Saturn from the receding Voyager 1

NASA / JPL-Caltech / Ted Stryk

Saturn from the receding Voyager 1

As I searched through the dataset, a group of images stood out. They were taken on November 13, 1980, a day after closest approach. None of the Narrow Angle Camera images contained Enceladus, but eight of the Wide Angle Camera images did. They showed the small crescent and night time hemisphere illuminated in Saturnshine as only a few pixels across.

Cleaned raw image from the dataset used

NASA / JPL-Caltech / Ted Stryk

Cleaned raw image from the dataset used

I thoroughly calibrated, deconvolved, and stacked the images. After combining different subsets as well as the full set, I am confident in the detection of the plumes, just where they should be.

Enceladus from Voyager 1 on November 13, 1980

NASA / JPL-Caltech / Ted Stryk

Enceladus from Voyager 1 on November 13, 1980

The right side is illuminated by the sun, the left by reflected light from Saturn, and the plume can be seen at the bottom.

In my excitement at having at last had some success with this project, I quickly wrote an Lunar and Planetary Science Conference abstract, which can be read here. It gives more detail about how this dataset was handled.

Erupting Enceladus over Saturn from Voyager 1

NASA / JPL-Caltech / Ted Stryk

Erupting Enceladus over Saturn from Voyager 1

On November 13, 1980, Voyager 1 captured Enceladus and Saturn. These images, processed by Ted Stryk over 35 years later, captured Enceladus' plumes—long before their discovery by the Cassini spacecraft.

I plan to continue sifting through images to see if there are other datasets worth processing in that way. I plan to do similar work with other worlds as well. At the very least, this indicates Enceladus is indeed constantly erupting, extending the baseline back more than two decades.

 

See other posts from February 2017


 

Or read more blog entries about: Enceladus, pretty pictures, amateur image processing, Voyager 1 and 2, Saturn's moons, many worlds, Saturn, explaining image processing

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Rays of Creusa


When viewed from a distance with the sun directly behind Cassini, the larger, brighter craters really stand out on moons like Dione. via NASA http://ift.tt/2kHYR3n

2017年2月20日 星期一

Almost Three Tails for Comet Encke


How can a comet have three tails? Normally, a comet has two tails: an ion tail of charged particles emitted by the comet and pushed out by the wind from the Sun, and a dust tail of small debris that orbits behind the comet but is also pushed out, to some degree, by the solar wind. Frequently a comet will appear to have only one tail because the other tail is not easily visible from the Earth. In the featured unusual image, Comet 2P/Encke appears to have three tails because the ion tail split just near to the time when the image was taken. The complex solar wind is occasionally turbulent and sometimes creates unusual structure in an ion tail. On rare occasions even ion-tail disconnection events have been recorded. An image of the Comet Encke taken two days later gives a perhaps less perplexing perspective. via NASA http://ift.tt/2m0u7dZ

TrumpSpace Update



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CRS-10 Mission in Photos (ongoing)

At 9:39:00 am ET on February 19, 2017, SpaceX’s Falcon 9 rocket, carrying the Dragon spacecraft, lifted off from Launch Complex 39A to deliver nearly 5,500 lbs of cargo and supplies to the International Space Station. This marked SpaceX’s first launch from Kennedy Space Center’s historic pad, and the first launch from LC-39A since July 8, 2011 when Atlantis lifted off for the final flight of the Shuttle Program.

Over the next two days, Dragon will conduct a series of height adjust and coelliptic burns to bring it closer to the International Space Station, culminating with capture of Dragon by the station’s robotic arm and berthing of the spacecraft to the Harmony module of the International Space Station. For about a month, crew members will unload the spacecraft and reload it with cargo to return to Earth.

Below is a summary of the mission in photos, with more hi res photos available on our Flickr site. You can also watch the archived webcast here, and find more information about the mission in our press kit.

Falcon 9, carrying the Dragon spacecraft, lifted off from Launch Complex 39A at Kennedy Space Center at 9:39:00 am ET, carrying nearly 5,500 lbs of cargo and supplies for the International Space Station.

The second stage engine nozzle glows amber following the successful separation of the Falcon 9 first and second stages. In this view, the Falcon 9 first stage is barely visible as a small white line perpendicular to the center of the second stage engine nozzle.

Grid fins are deployed to help orient the first stage during reentry; the second stage continues to carry Dragon to its intended orbit.

View from onboard camera of landing legs deployed just prior to touching down at Landing Zone 1.

Falcon 9 first stage after its first daytime landing at Landing Zone 1 in Cape Canaveral.

The Dragon spacecraft successfully separates from the second stage.

Dragon’s solar panels deploy and the spacecraft begins a series of height adjust and coelliptic burns to bring it closer to the International Space Station.



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Fact Checking ULA's Tweets



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Spitzer Discovered Something About Planets Somewhere

NASA to Host News Conference on Discovery Beyond Our Solar System

"NASA will hold a news conference at 1 p.m. EST Wednesday, Feb. 22, to present new findings on planets that orbit stars other than our sun, known as exoplanets. The event will air live on NASA Television and the agency's website. Details of these findings are embargoed by the journal Nature until 1 p.m."

Keith's note: Once again NASA is teasing us with some sort of important news about something. Of course the tabloids will immediately parse words, see words that NASA never used, and imagine that life has been found on other planets. Apparently Spitzer has something to do with this and there are some planets involved in this too. So I did a quick search for articles by the participants in this event as they relate to Spitzer. Have fun speculating.

- The Spitzer search for the transits of HARPS low-mass planets - II. Null results for 19 planets
- Illusion and Reality in the Atmospheres of Exoplanets
- Toward a Galactic Distribution of Planets. I. Methodology & Planet Sensitivities of the 2015 High-Cadence Spitzer Microlens Sample
- Searching For Rapid Orbital Decay of WASP-18b



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