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Ammonia Ice Clouds on Jupiter

The top cloud layer on Jupiter is thought to consist of ammonia ice, but most of that ammonia “hides” from spectrometers. It does not absorb light in the same way ammonia does. To many scientists, this implies that ammonia churned up from lower layers of the atmosphere “ages” in some way after it condenses, possibly by being covered with a photochemically generated hydrocarbon mixture. The New Horizons Linear Etalon Imaging Spectral Array (LEISA), the half of the Ralph instrument that is able to “see” in infrared wavelengths that are absorbed by ammonia ice, spotted these clouds and watched them evolve over five Jupiter days (about 40 Earth hours). In these images, spectroscopically identified fresh ammonia clouds are shown in bright blue. The largest cloud appeared as a localized source on day 1, intensified and broadened on day 2, became more diffuse on days 3 and 4, and disappeared on day 5. The diffusion seemed to follow the movement of a dark spot along the boundary of the oval region. Because the source of this ammonia lies deeper than the cloud, images like these can tell scientists much about the dynamics and heat conduction in Jupiter's lower atmosphere.

Release Date: October 9, 2007

Credit: NASA/Johns Hopkins University Applied Physics Laboratory/Southwest Research Institute


Source: NASA/JHUPL - New Horizons - Mission Photos
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Atmospheric Waves

With its Multispectral Visible Imaging Camera (MVIC), half of the Ralph instrument, New Horizons captured several pictures of mesoscale gravity waves in Jupiter’s equatorial atmosphere. Buoyancy waves of this type are seen frequently on Earth - for example, they can be caused when air flows over a mountain and a regular cloud pattern forms downstream. In Jupiter's case there are no mountains, but if conditions in the atmosphere are just right, it is possible to form long trains of these small waves. The source of the wave excitation seems to lie deep in Jupiter's atmosphere, below the visible cloud layers at depths corresponding to pressures 10 times that at Earth's surface. The New Horizons measurements showed that the waves move about 100 meters per second faster than surrounding clouds; this is about 25% of the speed of sound on Earth and is much greater than current models of these waves predict. Scientists can “read” the speed and patterns these waves to learn more about activity and stability in the atmospheric layers below.

Release Date: October 9, 2007

Credit: NASA/Johns Hopkins University Applied Physics Laboratory/Southwest Research Institute


Source: NASA/JHUPL - New Horizons - Mission Photos
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Atmospheric Structure

This image, which is a composite of images taken in several colors by the New Horizons Multispectral Visible Imaging Camera (MVIC), illustrates the remarkable diversity of structures in Jupiter's atmosphere. The image, whose colors are similar to what a voyager on New Horizons would see, is taken near the terminator, the boundary between day and night, and shows relatively small-scale turbulent polar structures as well as deep holes in the clouds and extended zonal structures at other latitudes. Data obtained from these and other New Horizons images taken during the encounter will provide valuable insight into the processes occurring on this gas giant.

Release Date: October 9, 2007

Credit: NASA/Johns Hopkins University Applied Physics Laboratory/Southwest Research Institute


Source: NASA/JHUPL - New Horizons - Mission Photos
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Changes on Io

A: A global map of Jupiter’s moon Io derived from eight images taken by the Long Range Reconnaissance Imager (LORRI) on the New Horizons spacecraft, as it passed Jupiter on its way to Pluto in late February 2007. Details as small as 12 kilometers (7 miles) are visible. The map shows the comprehensive picture of Io’s volcanism obtained by New Horizons. Yellow ovals denote areas with new, faded or shifted plume deposits since the last images taken by the Galileo spacecraft in 2001. Green circles denote areas where probable new lava flows have occurred. Cyan diamonds indicate locations of active volcanic plumes, and orange hexagons are volcanic hot spots detected by the Linear Etalon Imaging Spectral Array (LEISA) instrument. For plumes and hot spots, symbol size indicates the approximate relative size and brightness of the features.

B-F: Comparison of New Horizons (NH) and earlier images of major surface changes discovered by New Horizons at Io’s volcanoes Masubi (45 degrees S, 57 degrees West) and North Lerna (55 degrees S, 290 degrees W). The scale bars are 200 kilometers long, and a is the solar phase angle. At Masubi, old lava flows seen by Voyager and Galileo (B) have been obscured at low phase angles (C ) by deposits from two active plumes associated with a new 240-kilometer (150-mile) long dark lava flow, which is the longest lava flow known to have been erupted in the solar system since the discovery of Io volcanism in 1979. At North Lerna, a recent eruption has generated a 130-km long lava flow (F), as well as an active plume that has produced a concentric pattern of deposits.

This image appears in the Oct. 12, 2007, issue of Science magazine, in a paper by John Spencer, et al.

Release Date: October 9, 2007

Source: NASA/JHUPL - New Horizons - Mission Photos
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Io Eclipse Montage

New Horizons took this montage of images of Jupiter’s volcanic moon Io, glowing in the dark of Jupiter’s shadow, as the Pluto-bound spacecraft sped through the Jupiter system on Feb. 27, 2007.

(A): In this picture from the Long-Range Reconnaissance Imager (LORRI), dark blotches and straight lines are artifacts. The brightest spots (including the volcanoes Pele [P] and East Girru [EG]) are incandescent lava from active volcanoes. The more diffuse glows, and the many faint spots, are from gas in the plumes and atmosphere, glowing due to bombardment by plasma in Jupiter’s magnetosphere, in a display similar to the Earth’s aurorae. (B): The same image with a latitude/longitude grid, showing that the cluster of faint spots is centered near longitude 0 degrees, the point on Io that faces Jupiter. The image also shows the locations of the plumes seen in sunlit images (indicated by red diamonds), which glow with auroral emission in eclipse. (C ): Simulated sunlit view of Io with the same geometry, based on sunlit LORRI images. (D): A combination of the sunlit image (in cyan) and the eclipse image (in red), showing that all point-like glows in the eclipse image arise from dark volcanoes in the eclipse image. (E): This infrared image, at a wavelength of 2.3 microns, obtained by New Horizons Linear Etalon Spectral Imaging Array (LEISA) an hour after the LORRI image, showing thermal emission from active volcanoes. Elongation of the hot spots is an artifact. (F): Combined visible albedo (cyan) and LEISA thermal emission (red) image, showing the sources of the volcanic emission. That most of the faint point-like glows near longitude zero, seen in visible light in images A, B, and D, do not appear in the infrared view of volcanic heat radiation, is one reason scientists believe that these glows are due to auroral emission, not heat radiation.

This image appears in the Oct. 12, 2007, issue of Science magazine, in a paper by John Spencer, et al.

Release Date: October 9, 2007

Source: NASA/JHUPL - New Horizons - Mission Photos
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Tvashtar Montage

The Tvashtar plume on Io, seen by the Hubble Space Telescope (HST) and by New Horizons.

(A): The image in which the plume was discovered, taken by HST in ultraviolet light on Feb. 14, 2007, at a wavelength of 260 nm. The red diamond indicates location of the Tvashtar hot spot seen later by New Horizons. (B): An HST image of Io and the Tvashtar plume seen against Jupiter; sulfur gas in the plume absorbs ultraviolet light, making the plume look reddish in this color composite. The composite is composed of images taken at 260 nm (blue), 330 nm (green), and 410 nm (red). Other images in this montage are in visible light from the Long-Range Reconnaissance Imager (LORRI). The scale bar is 200 kilometers long and the yellow star indicates the projected location of the hot spot at the Tvashtar plume source. The dashed line is the terminator, the line dividing day from night on Io. (C ): The highest-resolution view of the full plume, at a resolution of 12.4 kilometers (7.7 miles) per pixel and a solar phase angle of 102 degrees, showing the complex filamentary structure of the plume. The images are sharpened by un-sharp masking; the dark line at the edge of the disk is an artifact of this sharpening. (D): An image at 145-degree phase angle at 22.4 kilometers (13.8 miles) per pixel, showing the time variability of the details of the plume structure and its persistent bright top. (F-J): Sequence of frames at 2-minute intervals showing dynamics in the upper part of the plume (the source is on the far side of Io). Colored diamonds track individual features whose speeds, projected on the plane of the sky, are shown in (E).

This image appears in the Oct. 12, 2007, issue of Science magazine, in a paper by John Spencer, et al.

Release Date: October 9, 2007

Source: NASA/JHUPL - New Horizons - Mission Photos
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Jupiter-Io Montage

This is a montage of New Horizons images of Jupiter and its volcanic moon Io, taken during the spacecraft’s Jupiter flyby in early 2007. The Jupiter image is an infrared color composite taken by the spacecraft’s near-infrared imaging spectrometer, the Linear Etalon Imaging Spectral Array (LEISA) at 1:40 UT on Feb. 28, 2007. The infrared wavelengths used (red: 1.59 µm, green: 1.94 µm, blue: 1.85 µm) highlight variations in the altitude of the Jovian cloud tops, with blue denoting high-altitude clouds and hazes, and red indicating deeper clouds. The prominent bluish-white oval is the Great Red Spot. The observation was made at a solar phase angle of 75 degrees but has been projected onto a crescent to remove distortion caused by Jupiter’s rotation during the scan. The Io image, taken at 00:25 UT on March 1st 2007, is an approximately true-color composite taken by the panchromatic Long-Range Reconnaissance Imager (LORRI), with color information provided by the 0.5 µm (“blue”) and 0.9 µm (“methane”) channels of the Multispectral Visible Imaging Camera (MVIC). The image shows a major eruption in progress on Io’s night side, at the northern volcano Tvashtar. Incandescent lava glows red beneath a 330-kilometer high volcanic plume, whose uppermost portions are illuminated by sunlight. The plume appears blue due to scattering of light by small particles in the plume.

This montage appears on the cover of the Oct. 12, 2007 issue of Science magazine.

Release Date: October 9, 2007

Source: NASA/JHUPL - New Horizons - Mission Photos
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Io and Europa Meet Again

This beautiful image of the crescents of volcanic Io and more sedate Europa is a combination of two New Horizons images taken March 2, 2007, about two days after New Horizons made its closest approach to Jupiter. A lower-resolution color image snapped by the Multispectral Visual Imaging Camera (MVIC) at 10:34 universal time (UT) has been merged with a higher-resolution black-and-white image taken by the Long Range Reconnaissance Imager (LORRI) at 10:23 UT. The composite image shows the relative positions of Io and Europa, which were moving past each other during the image sequence, as they were at the time the LORRI image was taken.

The picture was one of a handful of the Jupiter system that New Horizons took primarily for their artistic (rather than scientific) value. This particular scene was suggested by space enthusiast Richard Hendricks of Austin, Texas, in response to an Internet request by New Horizons scientists for evocative, artistic imaging opportunities at Jupiter.

This image was taken from a range of 4.6 million kilometers (2.8 million miles) from Io and 3.8 million kilometers (2.4 million miles) from Europa. Although the moons appear close together in this view, a gulf of 790,000 kilometers (490,000 miles) separates them. Io’s night side is lit up by light reflected from Jupiter, which is off the frame to the right. Europa's night side is dark, in contrast to Io, because this side of Europa faces away from Jupiter.

Here Io steals the show with its beautiful display of volcanic activity. Three volcanic plumes are visible. Most conspicuous is the enormous 300-kilometer (190-mile) high plume from the Tvashtar volcano at the 11 o'clock position on Io’s disk. Two much smaller plumes are also visible: that from the volcano Prometheus, at the 9 o'clock position on the edge of Io's disk, and from the volcano Amirani, seen between Prometheus and Tvashtar along Io’s terminator (the line dividing day and night). The Tvashtar plume appears blue because of the scattering of light by tiny dust particles ejected by the volcanoes, similar to the blue appearance of smoke. In addition, the contrasting red glow of hot lava can be seen at the source of the Tvashtar plume.

The images are centered at 1 degree North, 60 degrees West on Io, and 0 degrees North, 149 degrees West on Europa. The color in this image was generated using individual MVIC images at wavelengths of 480, 620 and 850 nanometers. The human eye is sensitive to slightly shorter wavelengths, from 400 to 700 nanometers, and thus would see the scene slightly differently. For instance, while the eye would notice the difference between the yellow and reddish brown colors of Io's surface and the paler color of Europa, the two worlds appear very similar in color to MVIC's longer-wavelength vision. The night side of Io appears greenish compared to the day side, because methane in Jupiter's atmosphere absorbs 850 nanometer light and makes Jupiter-light green to MVIC's eyes.

Release Date: October 16, 2007

Source: NASA/JHUPL - New Horizons - Mission Photos
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The Guest Perspective: Data for the Next Generations


November 7, 2007

By Joe Peterson

New Horizons is about to enter hibernation for its long trip to Pluto. It will be deep in slumber, but not forgotten, and we’ve taken a crucial step to ensure that its precious data will never be forgotten either. All planetary missions undergo a process called "data archiving," which protects the information against the ravages of time.

These archives have proven their value -- for example, scientists are still using data archives from the Voyager missions of the 1970s. The concept of archiving is simple, but to do it right, there is much to be considered.

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The New Horizons Science Operations Center at Southwest Research Institute,
Boulder, Colorado.
Click on image to view larger version.


Preserving data for the future is a challenge for everyone. Many of us have old floppy disks containing documents we'd like to be able to use at some point, but what will happen when we try to load those documents in 2010, especially if some of files were written with programs from 1995? Most of today’s computers don't have a floppy drive, and even if they did, we cannot be sure the old disks have not degraded or that modern software can still read the files they contain.

The people in charge of NASA’s Planetary Data System (PDS), where archives of data from missions like New Horizons are kept, worry about exactly this kind of thing every day. The periods over which scientists will want to study spacecraft data are very long. Therefore, the PDS wants to guarantee that data gathered today will last at least 50 or 100 years. No one knows what computers will be like that far into the future, but at PDS, it is routine to think ahead -- way ahead -- and they strive to make sure nothing will prevent long-term use of the planetary data entrusted to them.

New Horizons gathered some absolutely breathtaking images and other data during its Jupiter encounter earlier this year, but we cannot know exactly how this information will be valuable to a scientist 100 years from now. Archiving it properly is a real challenge, one that the New Horizons Science Operations Center has recently undertaken, resulting in our first PDS archive, a kind of "time capsule" that is designed to last into the distant future. All told, our archives include about 13,000 data files – including images and other data – adding up to about 54 gigabytes.

Useful Records

Creating a truly useful archive depends on several things. First of all, the physical media has to remain readable over many years. It would be a tragedy to take the archive off the shelf in 2050 and find that the data has all "flaked" off of the disks. Careful choices need to be made. Floppy disks, for many reasons, would be a poor choice - their capacity is low and they are too fragile, easily destroyed by magnets, fingerprints, dust, temperature extremes, and the like. The current "standard" media is CD-ROMs or DVD data discs. If you really want to be safe, CDs are a good bet, since they have stood the test of time very well so far. But when there is a lot of data, DVDs are a valid choice. The PDS can say "no" to any medium it thinks might be risky, as the consequences of lost data are dire.

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The New Horizons data collection includes hundreds of
images from the spacecraft's flight through the Jupiter
system, including this Long Range Reconnaissance
Imager (LORRI) photo of the moon Io peeking out
from behind the giant planet. More photos are
available in the Science Operations Center's LORRI
gallery
.



Next, the format of the data is important. In general, transparent, non-proprietary formats are best. For example, PDS does not consider word processing programs (such as Microsoft Word) to be a "safe" format. The specifications of the formats are not openly published, so if the company that sells and supports the software were to cease to exist in 100 years, or even if the version of program used to write the file became archaic, it would be difficult to open such files. So if you include a document in Word, you had better also include it in plain text; it is assumed that the scientists of the future will at least be able to make sense of regular ASCII bytes. As for visual elements such as figures and illustrations, the PDS allows these to be included as individual images. As you can see, creating such a "future proof" archive is not easy, and it takes a lot of work. The PDS even prohibits using conventions like very long filenames or those with mixed upper and lower-case letters even though today's computers can handle these. Part of ensuring compatibility is adhering to standards that have existed for quite some time.

Finally, an archive must have good documentation. We have to assume that future scientists will have no prior knowledge about the archive's contents, so to understand what a spacecraft sent back to Earth, it is vital to know how the spacecraft and its instruments worked, how the data was calibrated, and even what the data means. It is more than likely that the people who worked with the data when it was gathered (and therefore knew it very well) will be long gone, so the archive must stand on its own. This is one reason why the PDS insists that the archives be reviewed carefully by people who are independent of the mission. We at the New Horizons Science Operations Center have just gone through this review process, and I can tell you that it is absolutely rigorous, ensuring the data is usable by the widest audience possible.

Checking on Changes

Thanks to our PDS archive – coming soon to the PDS Web site – the New Horizons data will be available far into the future. Over the years, humans will surely want to look at what New Horizons has seen, prompted by either an expanded understanding of how our solar system works or simply the desire to see how things have changed in our little region of the universe.

Joe Peterson is manager of the New Horizons Science Operations Center at Southwest Research Institute, Boulder, Colo.

Source: NASA/JHUPL - New Horizons
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Autumn 2007: Onward to the Kuiper Belt


November 20, 2007

New Horizons has now covered 85% of the distance from the Sun to Saturn’s orbit, which it will pass in mid-2008. Of course, Saturn will be nowhere near New Horizons when we pass that milestone, as it is by chance located far around the Sun from the path New Horizons is following to Pluto. But as you can tell, we are really getting to be well into the outer solar system now.

Since I last wrote you, in early October, the New Horizons team has been busy on two major fronts. One of these has been planning and executing our 2007 Annual Checkout (ACO) of the spacecraft and its payload. As our first ACO, this three-month operation has been a pathfinder for the team, teaching us how to make improvements for subsequent ACOs in 2008, 2009 and beyond.

The other front we’ve been working on is Pluto encounter planning. As I’ve written here before, we are planning for Pluto now, to take advantage of the experienced team that took us through our virtually flawless Jupiter encounter earlier this year.

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Budget constraints will force us to slim down the team in mid-2009, so we need to finish the Pluto planning before many of the Jupiter encounter team members move on to other projects.

Our first Annual Checkout just wrapped up, after more than 500 separate spacecraft and instrument activities; and it was a great success. We also used the data gathered to recalibrate our instruments — something we’ll do several times as we fly out to the Pluto system. As you know from my last posting here, we also planned and successfully accomplished an engine burn during ACO-1. This maneuver refined our course and dramatically narrowed our expected trajectory errors at Pluto.

We did have a couple of unexpected events during ACO-1. One came in early October, when the spacecraft partially lost track of its timeline owing to a very subtle kind of error generated by a command script we’d sent it. The operations team caught this and recovered from it very quickly. It was really a blessing that this subtle behavioral flaw manifested itself now, rather than at Pluto, so we can protect against it. It’s these kinds of idiosyncrasies that our testing and flight operations hope to expose. So, despite the fact it cost us some lost sleep and some cruise science observations, we’re very glad to have learned this lesson.

The second unexpected event came just last week, on November 12, when a cosmic ray or some other kind of charged particle caused our main computer to reboot. This is the fourth such computer reboot we have had in flight caused by space radiation bursts. Preflight predictions were for these events to be far more rare than this, and our engineering team is looking into why this is occurring more often than predicted. Fortunately, on the four occasions this occurred, the onboard spacecraft autonomy software performed as planned and recovered New Horizons safely.

The third and final such event took place on November 16, when the spacecraft’s main computer executed a power on reset (POR) because of a glitch on its power line. Since this was so unexpected, we are analyzing what happened and have decided not to enter hibernation until late December while we analyze the root cause of this anomaly and put in place some software protection against future events. For the next couple of weeks, we’ll monitor the spacecraft three to four times a week using NASA’s Deep Space Network to collect more data.

Then, between December 11 and 17, the spacecraft will pass near the Sun as seen from Earth. (Don’t worry, New Horizons really is out in the frigid cold near Saturn, it just appears to be near the Sun when seen from Earth’s vantage point.) This event is called “solar conjunction” and it occurs every year as the Earth itself reaches a point nearly opposite the Sun from New Horizons. As during last year’s solar conjunction, we will lose contact with New Horizons due to radio interference from the Sun, which will be just one to three degrees away from New Horizons and in our tracking antennas’ field of view.

December 17, the day we exit this year’s solar conjunction, is an anniversary for us; on that day in 2005, New Horizons was lifted onto its Atlas launch vehicle down in Florida. It’s a nice coincidence to note that precisely 102 years before that day, in 1903, the Wright brothers made their first flight at Kitty Hawk.

As we exit solar conjunction on December 17, we’ll have a fairly intense week of activity. During that week we will re-point our dish antenna to better position it for communications with Earth and play back recorded engineering and Student Dust Counter detector telemetry. The team will also prepare the spacecraft for a long period of hibernation that will begin on December 23 and continue uninterrupted (we hope!) until next May, when we next break hibernation for about a week to reposition our antenna again for better communications with Earth. We’ll use that operations opportunity in May to send home some of the lower priority “cruise science” data taken this month that couldn’t be squeezed down during ACO-1. Then, we’ll go back to silent running until ACO-2 begins late next September.

During the almost 40 weeks we’ll be in hibernation in 2008, we won’t be sending commands to the spacecraft. But we will check its health via weekly beacon tones and (beginning in early 2008) monthly telemetry sessions. Many of you may notice that this is a less frequent set of checks than we performed in 2007. That’s because as we gain experience with the spacecraft in hibernation mode, we can reduce the oversight we perform on it. This “lengthening of the leash” as I like to call it, is something we have planned for years. And unless something untoward occurs, this pace of weekly beacon tone and monthly telemetry checks is how we will run hibernation activities in future years on the way to Pluto.

That’s my update on mission activities for now, but before I close I’d like to show you two things related to the Pluto encounter we are now beginning to plan.

Figure 1 shows the “block schedule” that defines our Pluto system encounter phases. By studying this figure you will see that we plan to begin the encounter operations about six months before reaching Pluto, and we do not finish — including all of the data transmissions and plasma and dust environment measurements — until six months after the July 14 encounter itself. Of course, most of the action occurs in the roughly two-month period centered on encounter day, when our resolution and sensitivity are dramatically better than anything Earth-based and Earth-orbiting telescopes can match.

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New Horizons’ encounter with the Pluto
system will span a year, in which there will
be three successively closer approach phases
(APs 1, 2 and 3), a near encounter phase
(NEP) lasting two days, which will be followed
by three successively more distant departure
phases (DPs 1, 2 and 3).
Click on the image to see a larger version.



Figure 2 provides a view of the Pluto system at our moment of closest approach. It shows where the spacecraft will be at its moment of closest approach to Pluto, relative to Pluto and all three of Pluto’s satellites, i.e., at the green “+” symbol. As you can see, we will be 13,700 kilometers from Pluto’s center and therefore 12,500 kilometers from its surface. You can also see that Nix and Charon are arrayed on different sides of the spacecraft at roughly similar distances, but Hydra is considerably farther away, off in the rough direction that Charon will appear to be.

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The geometry of Pluto and its three satellites
– Charon, Nix and Hydra – are shown here
relative to our spacecraft aim point (the green “+”)
at the moment of closest approach (C/A) to Pluto.
Click on the image to see a larger version.


In the coming year while our beauty sleeps, we will plan this encounter in great detail, leading up to a full suite of rehearsals on our mission simulator in 2009, which will in turn lead to rehearsals on New Horizons itself in 2010. As 2008 unfolds, I’ll keep you apprised of many of the interesting things we plan to do during the Pluto encounter and how we plan to do them.

Well, that catches you up with where New Horizons is and what the spacecraft and project team have been doing. I’ll be back with more news around the start of the new year. In the meantime, keep on exploring, just like we do!

- Alan Stern

Source: NASA/JHUPL - New Horizons
magnetar
I just have to respond. This is a very surprising section. Look at those images! Look at how this shoestring project is starting to amaze.

If only we had allowed a better budget. These people are really making the most out of this mission. Oh, the possibilities. And it could be so, with honest tax money. That's how it should be.

Going to the outer planets just fires the imagination. I think Neptune would be an awesome sight to see.

So, thanks for these updates.






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Headlines

January 15, 2008

'Ice' Congratulates 'Fire' on a Successful Mercury Flyby

The New Horizons Pluto-Kuiper Belt exploration team sends hearty congratulations to its colleagues on the MESSENGER mission, who orchestrated an historic flyby of the planet Mercury on Jan. 14.

The New Horizons and MESSENGER spacecraft – both built and operated by the Johns Hopkins University Applied Physics Laboratory (APL) in Laurel, Md. – make up NASA’s “Fire and Ice” tandem, set out to explore the extreme frontiers of the solar system. New Horizons is two years into its decade-long voyage to Pluto and the frozen, rocky environs of the distant Kuiper Belt. Headed in the opposite direction, MESSENGER will be the first spacecraft to orbit the Sun’s closest planetary neighbor.

“From one mission of pioneering exploration to another, congratulations to the MESSENGER team!” says New Horizons Principal Investigator Alan Stern, of NASA Headquarters.

MESSENGER will fly by Mercury two more times before settling into a yearlong orbit around the planet in March 2011. It’s only the second spacecraft to even fly past the innermost planet, and is gathering data on parts of Mercury’s surface the first visitor, NASA’s Mariner 10, couldn’t see when it sped by three times in the mid-1970s.

“The New Horizons team shares the excitement about the new knowledge that MESSENGER will provide about Mercury,” says Glen Fountain, New Horizons project manager at APL.

Check out the latest images and news from MESSENGER at _http://messenger.jhuapl.edu.

Source: NASA/JHUPL - New Horizons - News
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Happy Birthday New Horizons!
Two Years on the Road to the Ninth Planet


January 17, 2008

Just like the parent of a kid growing up from an infant to a toddler, my experience with New Horizons in flight – since our launch two years ago this week – is that the first two years have passed amazingly quickly and yet amazingly slowly, all at the same time. I guess that given some of the spacecraft hiccups of the past several months, one could also analogize that New Horizons has reached the “Terrible Two” stage and is into saying “no” a little more these days than in its first year.

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New Horizons celebrates the completion of
its second year in flight this Saturday, January 19.


Honestly, though, it’s been a great second year that included a phenomenally successful Jupiter encounter, a course correction, our first annual checkout, and science team work to begin in earnest the planning for the encounter at Pluto, still seven years hence. (Interestingly, this month also commemorates the seventh anniversary of the first New Horizons team meetings to write our proposal to NASA, so we are now at the halfway point from project inception to encounter!)

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This montage of giant Jupiter and its volcanic
moon Io, replete with the spectacular Tvashtar
polar plume, was assembled from New Horizons
imagery.


As you can see by visiting our Where Is New Horizons, we are now nearing a distance of 9 Astronomical Units from the Sun and speeding onward. This time next year, we’ll already be almost halfway between 12 and 13 AU!

Our spacecraft will be in quiet cruise or hibernation for most of 2008. Short wakeups will occur in May and December to re-point our high-gain antenna toward Earth and conduct other maintenance activities. Also on our flight plan is our second active checkout, which will fill the period from September through early November with many kinds of spacecraft and instrument activities. But otherwise we plan for things to be very quiet on orbit this year. And we have already determined from tracking data that our trajectory correction maneuver in late September was so accurate that no clean-up burn will be required in 2008 (nor will such be very likely in 2009, either).

The major work of New Horizons in 2008 will be on the ground. One activity will be the creation, testing and uploading of new spacecraft software with various bug fixes and performance improvements that derived from our Jupiter encounter and second-year flight experiences. Another large activity will be designing and building the entire Pluto near-encounter sequence, which we will also prepare for test on our spacecraft simulator, “NHOPS,” next year. In addition to these two activities and routine flight operations in cruise and annual checkout, we also expect to commission NHOPS-2, our newly minted backup spacecraft simulator.

In the meantime, though, we’ve savoring the successful second year of flight the project has had. And the homemade cake below (made by APL’s Simmie Berman) is evidence of that!

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Well, that catches you up with where New Horizons is and what the spacecraft and project team have been doing. I’ll be back with more news in March. In the meantime, keep on exploring, just like we do!

- Alan Stern

Source: NASA/JHUPL - New Horizons
magnetar
The story of hard work and determination that went in to this project is impressive.

Thanks for the update, and fascinating image from Jupiter.
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Headlines

January 24, 2008

A Hi-Def Peek at Pluto

New Horizons made its first detection of Pluto using the high-resolution mode of its Long Range Reconnaissance Imager (LORRI) during three separate sets of observations in October 2007.

“LORRI first detected Pluto in September 2006 in its low-resolution format,” says New Horizons Principal Investigator Alan Stern, of NASA Headquarters, “but this time around we were able to take longer exposures and to detect Pluto using a camera resolution that is four times better than before.”

New Horizons was still too far from Pluto (3.6 billion kilometers, or 2.2 billion miles) for LORRI to resolve any details on Pluto’s surface – that won’t happen until summer 2014, approximately one year before closest approach. For now the entire Pluto system remains a bright dot to the spacecraft’s telescopic camera, though LORRI is expected to start resolving Charon from Pluto – seeing them as separate objects – in summer 2010.

During the October 2007 observations, Pluto was located in the constellation Serpens, in a region of the sky dense with background stars. “Using LORRI’s high-resolution mode allowed us to more easily pick out Pluto in a virtual sea of surrounding stars,” says New Horizons Project Scientist Hal Weaver of the Johns Hopkins University Applied Physics Laboratory (APL), which provided the LORRI instrument.

Marking another first for New Horizons, LORRI also detected clear variations in Pluto’s brightness. Pluto rotates on its axis once every 6.4 days, allowing observers to see different portions of the planet’s surface (i.e., different longitudes). From ground-based and Hubble Space Telescope observations scientists have seen repeatable, well-defined differences in Pluto’s brightness they believe is caused by variations in frost cover over its surface. New Horizons will determine whether that is indeed the correct explanation when the spacecraft flies by Pluto in July 2015.

“In the meantime, it’s gratifying to see that New Horizons itself now has the capability to track Pluto’s brightness variations over the next seven and a half years, and from a slightly different perspective than what we normally see from Earth,” Weaver says.


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This image demonstrates the first detection of Pluto using LORRI’s high-resolution mode, which provides a clear separation between Pluto and numerous nearby background stars. Typically, LORRI’s exposure time in hi-res mode is limited to approximately 0.1 seconds, but by using a special pointing mode that allowed an increase in the exposure time to 0.967 seconds, scientists were able to spot Pluto, which is approximately 15,000 times fainter than human eyes can detect.

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This montage shows the effects of using different resolutions and exposure times during LORRI observations of Pluto on October 6, 2007. The top left image was taken with LORRI in high-resolution mode using an exposure time of 0.967 seconds. The image to its right had the same exposure time but was taken in LORRI’s low-resolution mode with pixels that are four times larger, which makes the stars and Pluto look “fatter” and, therefore, less distinct. The image to the lower left is another LORRI image taken in low-resolution mode, but with an exposure time that is four seconds longer, which allows us to see “deeper” and pick up even fainter stars. (Pluto is clearly detected and is circled in each of these LORRI images.) The lower right image is a digitized photographic plate of the same portion of the sky taken in July 1986 by a large telescope in Australia for the Palomar Sky Survey. Pluto is not in this image, but Pluto’s location in the October 2007 observations is indicated by the small red circle. This image captures stars that are approximately 40 times fainter than can be seen in the lower left LORRI image and illustrates the richness of the background star field in this region of the sky.


Source: NASA/JHUPL - New Horizons - News Center
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Gallery: Science Photos

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Pluto in Hi-Def
Release Date:
Jan 24, 2008

This image demonstrates the first detection of Pluto using the high-resolution mode on the New Horizons Long-Range Reconnaissance Imager (LORRI). The mode provides a clear separation between Pluto and numerous nearby background stars. When the image was taken on October 6, 2007, Pluto was located in the constellation Serpens, in a region of the sky dense with background stars.

Typically, LORRI’s exposure time in hi-res mode is limited to approximately 0.1 seconds, but by using a special pointing mode that allowed an increase in the exposure time to 0.967 seconds, scientists were able to spot Pluto, which is approximately 15,000 times fainter than human eyes can detect.

New Horizons was still too far from Pluto (3.6 billion kilometers, or 2.2 billion miles) for LORRI to resolve any details on Pluto’s surface – that won’t happen until summer 2014, approximately one year before closest approach. For now the entire Pluto system remains a bright dot to the spacecraft’s telescopic camera, though LORRI is expected to start resolving Charon from Pluto – seeing them as separate objects – in summer 2010.

Credit: NASA/Johns Hopkins University Applied Physics Laboratory/Southwest Research Institute

Source: NASA/JHUPL - New Horizons - Science Photos
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Headlines

For Release: February 21, 2008

New Horizons Crosses 9 AU

New Horizons passed a planetary milepost today at 5 a.m. EST when it reached a distance of 9 astronomical units (AU) from the Sun – about 836.6 million miles, or nine times the distance from the Earth to the Sun. “The spacecraft destined for the ninth planet is now just beyond 9 AU and continuing outbound for the solar system’s frontier at more than 60,000 kilometers per hour!” says New Horizons Principal Investigator Alan Stern, of NASA Headquarters.

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New Horizons has covered nearly 970.5 million miles (1.56 billion kilometers) since its launch from Cape Canaveral Air Force Station, Fla., on January 19, 2006. Speeding toward Pluto at about 42,000 miles (67,500 kilometers) per hour, New Horizons will zip past the orbit of Saturn – where the Cassini spacecraft now operates – on June 8. That crossing will make New Horizons the farthest spacecraft on its way to or at its primary target.

New Horizons itself won’t have long to enjoy this latest accomplishment, though, as mission operators will put the spacecraft into regularly scheduled hibernation this afternoon at 3:50 p.m. EST.

Source: NASA/JHUPL - New Horizons - News
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Headlines

For Release: February 28, 2008

Memories of Jupiter

A year ago, New Horizons was flying through the heart of the Jupiter system, gradually picking up speed and systematically gathering spectacular data on the solar system’s largest planet and its closest moons. The results of that spectacular flyby have since been featured on thousands of electronic and printed pages, including a special issue of the journal Science in October 2007.

New Horizons scientists recently took a new look at one of the more memorable images from the Jupiter collection: that of the erupting volcano Tvashtar on the moon Io. Taken through two of the four filters in the sensitive Multispectral Visible Imaging Camera, the picture shows the reddish colors of the plume deposits surrounding the base of the volcano – a view we hadn’t seen in earlier pictures. Check it out in the New Horizons gallery.

Revisit the highlights of the historic Jupiter encounter:

New Horizons Sees Changes in Jupiter System, October 2007

Pluto-Bound New Horizons Provides New Look at Jupiter System, May 2007

Source: NASA/JHUPL - New Horizons - News
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Headlines

For Release: February 28, 2008

Seeing Red

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This New Horizons image of Jupiter's volcanic moon Io was taken at 13:05 Universal Time during the spacecraft's Jupiter flyby on February 28, 2007. It shows the reddish color of the deposits from the giant volcanic eruption at the volcano Tvashtar, near the top of the sunlit crescent, as well as the bluish plume itself and the orange glow of the hot lava at its source. The relatively unprocessed image on the left provides the best view of the volcanic glow and the plume deposits, while the version on the right has been brightened to show the much fainter plume, and the Jupiter-lit night side of Io.

New Horizons' color imaging of Io’s sunlit side was generally overexposed because the spacecraft's color camera, the super-sensitive Multispectral Visible Imaging Camera (MVIC), was designed for the much dimmer illumination at Pluto. However, two of MVIC's four color filters, the blue and "methane" filter (a special filter designed to map methane frost on the surface of Pluto at an infrared wavelength of 0.89 microns), are less sensitive than the others, and thus obtained some well-exposed views of the surface when illumination conditions were favorable. Because only two color filters are used, rather than the usual three, and because one filter uses infrared light, the color is only a rough approximation to what the human eye would see.

The red color of the Tvashtar plume fallout is typical of Io's largest volcanic plumes, including the previous eruption of Tvashtar seen by the Galileo and Cassini spacecraft in 2000, and the long-lived Pele plume on the opposite side of Io. The color likely results from the creation of reddish three-atom and four-atom sulfur molecules (S3 and S4) from plume gases rich in two-atom sulfur molecules (S2 After a few months or years, the S3 and S4 molecules recombine into the more stable and familiar yellowish form of sulfur consisting of eight-atom molecules (S8), so these red deposits are only seen around recently-active Io volcanos. Though the plume deposits are red, the plume itself is blue, because it is composed of very tiny particles that preferentially scatter blue light, like smoke. Also faintly visible in the left image is the pale-colored Prometheus plume, almost on the edge of the disk on the equator at the 9 o'clock position.

Io was 2.4 million kilometers from the spacecraft when the picture was taken, and the center of Io's disk is at 77 degrees West longitude, 5 degrees South latitude. The solar phase angle was 107 degrees.

Credit: NASA/Johns Hopkins University Applied Physics Laboratory/Southwest Research Institute.

Source: NASA/JHUPL - New Horizons - News
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Green Beacons for a Golden Bird


May 17, 2008

As you read these words, the New Horizons spacecraft remains in a long period of almost continuous hibernation, which began on Feb. 21 and stretches until Sept. 2. During this time the spacecraft will fly from nine to almost 11 times as far from the Sun as the Earth is, covering more than 300 million more kilometers! Except for two weeks of high activity that begins May 20, the spacecraft is running on its own, and doing little besides reporting its status each Monday and delivering a brief telemetry report most Thursdays. These contacts have shown that things are going well: all of the weekly status reports (technically called “beacon tones”) have been green, and all of the telemetry passes have indicated that the spacecraft is performing well.

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New Horizons, with its golden Mylar thermal covering,
goes through preflight preparations at NASA’s Kennedy
Space Center.
(Click for larger image)


lthough our spacecraft has been hibernating, our ground and science teams are anything but quiescent.

Planning for the Pluto encounter is in full swing. Our goal is to complete the near-encounter sequence design and testing within a year, so that we can conduct a full rehearsal on New Horizons in mid-2009. In fact, just this week we completed an Encounter Requirements Review to verify that, before we begin designing the detailed encounter sequences, we have a complete list of every scientific and navigation activity that we plan to conduct during the encounter. In June we will conduct an Encounter Feasibility Review, in which detailed encounter plans will be tested against dozens of ground and spacecraft constraints – such as power, data storage and available fuel – to ensure that each aspect of those plans is feasible. We’ll follow that review with a Preliminary Design Review in August, after which detailed sequence building will get under way.

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Large antennas like this one in Canberra,
Australia, form the Deep Space Network
(DSN) that NASA uses to track missions
beyond Earth orbit. In addition to transmitting
commands and receiving telemetry from
New Horizons, this particular antenna will
be used on July 14, 2015, to generate the
radio occultation signal that our spacecraft
will use to probe the temperature and
pressure of Pluto’s atmosphere.


July 2015 may be seven years away, but with our need to reduce our team size and budget after 2009, New Horizons must complete its encounter planning, ground testing, and a full dress rehearsal on the spacecraft barely more than one year from now!

The New Horizons team is also busy planning sequences for this fall’s spacecraft and instrument checkout period, which will run from Sept. 2 to mid-November. In addition to the annual tests, this fall’s activities will also include uplinking new command and data handling, guidance/navigation, and fault protection software that resolves several dozen minor bugs and provides new capabilities that will improve our ability to perform at Pluto and in the Kuiper Belt. The team is nearly finished building and beginning to test “NHOPS II,” our second (and long desired) backup New Horizons spacecraft simulator, which will be operational at the Johns Hopkins Applied Physics Lab (APL) by late summer.

I mentioned our plan to wake up New Horizons for a couple of weeks beginning on May 20; the main reason for the wake-up is to reposition the spacecraft antenna to account for the motion of Earth around the Sun. We have to do this several times each year, and we use it as an opportunity to combine important activities that need to occur between annual checkouts.

This time, spacecraft activities will include navigation ranging tests that mimic Pluto operations; spacecraft tracking; downlinking data that the Venetia Burney Student Dust Counter instrument has collected this year; a “bug fix” software upload and subsequent test of the SWAP solar wind plasma instrument; and an upload of the spacecraft command sequence that will guide New Horizons from June 3 to Sept. 5.

Bon Voyage, Jo-Anne!

The last thing I’ll mention is that our project secretary, Jo-Anne Kierzkowski, retired a couple of weeks ago. JoAnne worked at APL for many years, and had been with the New Horizons project since our team formed in December 2000.

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Everyone on New Horizons will miss our
retiring secretary, Jo-Anne Kierzkowski,
who began with the project team at its
inception in late 2000.


Jo-Anne provided us with expert project coordination, from the start of our proposal writing, through spacecraft design, build, test and launch, and the first 1.5 billion kilometers of travel toward Pluto. Although she isn’t going far and will be celebrating with us at the Pluto encounter in 2015, we will miss her work and her cheerful smile every day in between.

Well, that catches you up with where New Horizons is and what the spacecraft and project team have been doing. I’ll be back with more news soon. In the meantime, keep on exploring, just like we do!

- Alan Stern

Source: NASA/JHUPL - New Horizons
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Headlines

May 29, 2008

Milestones Ahead: New Horizons Set to Cross Saturn’s Orbit
Spacecraft Will Be First to Journey beyond Ringed Planet Since 1981

Last week, New Horizons woke up from its longest electronic hibernation period to date — 89 days. And over the next 10 days, the New Horizons team will celebrate a trio of milestones on the spacecraft’s long journey to explore Pluto in 2015.

The team roused New Horizons from hibernation mainly to re-point the spacecraft’s antenna, adjusting to the changing position of Earth around the Sun. The operations team is also carrying out navigation-ranging tests that mimic operations at Pluto, as well as conducting additional tracking, downlinking data from the student dust counter instrument, installing and testing bug-fix software for the SWAP solar wind plasma instrument, and uploading the spacecraft flight plan for the next several months. These activities will be complete by June 2; the next day, New Horizons will re-enter electronic hibernation for another 91 days. It will awaken for its annual checkout on Sept. 2.

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New Horizons is quickly approaching Saturn’s orbit.

New Horizons reaches the first milestone just before going back into hibernation. On June 2, the spacecraft will be 10 Astronomical Units (AU) from the Sun. One AU is the distance from the Earth to the Sun, about 93 million miles (or 149 million kilometers). New Horizons will be 930 million miles, or just about 1.5 billion kilometers from the Sun.

On June 3, the mission team will celebrate the spacecraft’s 866th day in flight – or one-quarter of its 3,463-day (9.5-year) journey to Pluto. New Horizons will pass its halfway mark to Pluto in another 866 days, on Oct. 17, 2010.

Most notably, however, on Sunday, June 8, the spacecraft will cross the orbit of Saturn, though Saturn itself is nowhere near the course New Horizons is following to Pluto. “This milestone is significant because the last time any spacecraft journeyed beyond Saturn was 27 years ago, in August 1981, when Voyager 2 passed Saturn on its way to encounters with Uranus and Neptune later in the 1980s,” says New Horizons Principal Investigator Alan Stern.

After New Horizons passes the distance where NASA’s Cassini orbiter is operating at Saturn, only two spacecraft will be operating farther out than the Pluto-bound probe. These are NASA’s Voyagers 1 and 2, which are at the edge of the Sun’s heliosphere approximately 100 AU away.

To continue tracking New Horizons on its voyage across the solar system toward Pluto and the frontier worlds of the Kuiper Belt, check in at http://www.pluto.jhuapl.edu/mission/whereis_nh.php.

Source: NASA/JHUPL - New Horizons - News
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Headlines

June 8, 2008

New Horizons Ventures Beyond Saturn’s Orbit

New Horizons crossed the orbit of Saturn on June 8, passing yet another interplanetary milepost on its voyage to Pluto and the icy environs of the Kuiper Belt.

Spinning is healthy in electronic hibernation, New Horizons reached a distance of 10.06 astronomical units (about 935 million miles or 1.5 billion kilometers) from the Sun at 10:00 universal time, becoming the first spacecraft to journey beyond Saturn’s orbit since Voyager 2 passed the ringed planet nearly 27 years ago. In fact, Voyager 1 and 2, at the edge of the Sun’s heliosphere some 100 AU away, are the only spacecraft operating farther out than New Horizons.

New Horizons reached Saturn's distance just two years and four months after launch - by far a faster transit to Saturn than any previous spacecraft. (Voyager 1, the previous record holder, made the trip in approximately three years and two months.)

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New Horizons Passing the Orbit of Saturn.

New Horizons has crossed the orbits of three planets since its launch in January 2006, though only one – Jupiter, in February 2007 – was close enough for a gravity boost and for the spacecraft to study. Saturn is more than 1.4 billion miles (2.3 billion kilometers) from New Horizons at present.

Healthy and “resting” after a productive two-week series of system checks, maintenance activities, and software and command uploads,the spacecraft is humming through the outer solar system at 40,850 miles (65,740 kilometers) per hour. The New Horizons team expects to keep the spacecraft in hibernation until Sept. 2. Next checkpoint on New Horizons' journey is the orbit of Uranus, which it crosses on March 18, 2011.

Source: NASA/JHUPL - New Horizons - News
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Headlines

July 2, 2008

New Horizons Team Celebrates 30th Anniversary of Charon’s Discovery

This week the New Horizons mission team celebrates the 30th anniversary of the discovery of Pluto’s largest and first moon, Charon, by U.S. Naval Observatory astronomers James Christy and Robert Harrington.

Charon, whose discovery was officially announced on July 7, 1978, orbits nearly 11,390 miles (about 18,220 kilometers) from Pluto’s surface and has a diameter of about 750 miles (1,210 kilometers). At half the diameter of Pluto, Charon is the largest moon relative to its planet in our solar system.

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Charon discovery image, 1978.

Charon’s surface is covered in water ice, and its interior is known to be a nearly even combination of rock and water ice. Unlike Pluto, it has no substantial atmosphere. “The historic discovery of Charon ushered in the modern understanding of Pluto as a double planet and the product of a giant collision that formed the system in much the same way as the Earth-moon system was formed,” says New Horizons Principal Investigator Alan Stern.

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Artist's impression of Charon (right) and Pluto.

The Pluto family grew just three years ago, when Stern and New Horizons Project Scientist Hal Weaver led a team that discovered two additional, much smaller moons, later named Nix and Hydra.

New Horizons is en route to fly by and reconnoiter the Pluto system seven years from now, in July 2015, turning these moons and their parent planet from points of light into well-mapped worlds.

Read more about Charon’s discovery in our Science section or on the U.S. Naval Observatory Web site.

Source: NASA/JHUPL - New Horizons - News
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Journeying Beyond Saturn


July 29, 2008
As avid followers of New Horizons know, our spacecraft has been mostly hibernating since February, and will continue to so do until Sept. 2, when we will wake it to begin its second annual checkout. Many of you will also recall that New Horizons passed the orbit of Saturn in early June. New Horizons is the first spacecraft to venture this far (a billion kilometers from the Sun!) since the last of the Voyagers accomplished the same milestone in the summer of 1981. We are now nearly 96 million kilometers (60 million miles) beyond Saturn, and will cross the orbit of Uranus – about 2 billion kilometers from the Sun – in March 2011.

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New Horizons passed the orbit of Saturn on June 8 and continues
on its way to exploring the last of the nine planets known prior to
the exciting discovery of many new, dwarf planets in the solar
system’s distant Kuiper Belt – our scientific destination.
(Credit: NASA)


My last PI Perspective detailed our plans to wake New Horizons up in late May for two weeks of onboard engineering activities. That brief wake-up went well; we re-pointed the antenna and loaded SWAP instrument software, among other accomplishments. We then put our spacecraft back into hibernation on June 3, right on schedule.

After that, we resumed our weekly Monday check-ins with the spacecraft to verify its health. In June, what had been our weekly Thursday telemetry (“TLM” on the mission calendar) contacts to monitor engineering during hibernation became every-other-Thursday events. As we gain experience in hibernation, our goal is to check this telemetry just once a month beginning in 2009 (though weekly beacon health-status checks will continue whenever we are in hibernation, right through 2015).

Of course, spaceflight isn’t as routine as other forms of flight, and that was re-emphasized to us on Monday, July 7, when our weekly beacon check-in revealed that New Horizons was transmitting a “red” (emergency) beacon instead of its familiar “green” (nominal flight) beacon. This told us that the spacecraft had experienced a significant anomaly in the past week. With the help of NASA’s Deep Space Network of tracking stations, our mission operations team immediately swung into action, contacting the spacecraft that evening and downloading telemetry diagnostics the next day. By mid-week our operations team had diagnosed the problem and had devised a recovery strategy. Our main flight computer had unexpectedly reset itself after becoming hung up in a software loop. By Friday, July 11, our operations and engineering teams had assessed this anomaly, determined that it was safe for the spacecraft to re-enter hibernation, and commanded New Horizons to do so.

In the three weeks since, New Horizons has hibernated uneventfully, sending green beacons every Monday while our spacecraft computer engineering team, led by Steve Williams of the Johns Hopkins University Applied Physics Laboratory, worked to diagnose why our main computer (called “C&DH-1”) had gotten itself hung up. Although this investigation is ongoing, we have held a review board and we are using test versions of the C & DH (Command and Data Handling) system to reproduce the failure here on the ground. I’ll update you on this when we know more.

As we continue out toward the Kuiper Belt, our flight plan for August is pretty boring, since we plan to hibernate throughout the month. The figure below summarizes that plan; in it you can see the Monday beacon passes (“Bea”) using one DSN station each for 1.5 hours, and the bi-weekly Thursday telemetry contacts that use a DSN antenna for eight hours. You can also see that the Venetia Burney Student Dust Counter (SDC) instrument will be taking data all month, as is normal during hibernation. Those with a sharp eye will notice an extra Thursday telemetry pass at the end of August; this is because we want to gather extra engineering data just before emerging from hibernation on Sept. 2. Some of you may also notice the code “SDC 005” on a few days near the end of August; this indicates a special internal calibration of the SDC we’ll perform when hibernation ends, to help with data analysis from the instrument.

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The August flight plan calendar for New Horizons as it continues in hibernation.

Like a kid returning to school in the fall, New Horizons gets busier after August. The plan for September-October-November involves a zoo of checkout activities, spacecraft tests, software updates, and instrument calibrations and tests that comprise our second ACO (“Annual Checkout”). ACO-1 was conducted last fall; we didn’t conduct one in 2006 because we were still commissioning the spacecraft and instrument payload in preparation for our early-2007 Jupiter flyby.

I’ll write more about ACO-2 in my next two updates, but just to give you a feel for how much more active the spacecraft will be, compare the September schedule (below) to the August schedule, and think about this: October will be busier still! As our spacecraft hibernates in August, our mission operations and science operations teams are planning and testing the detailed command sequences for ACO-2, which is, without doubt, an intensive, full-time job.

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The September flight plan calendar for New Horizons as it begins Annual Checkout 2
(ACO-2).


Pluto Science

Before I close, I want to tell you about two recent science results that relate to our main flyby target – the Pluto system – and give you a heads up on a cool new way to follow the progress of New Horizons.

The first of the two science results appears in the August Astronomical Journal, in a paper by Bradley Shaffer of Louisiana State University and a host of co-workers from various institutions. Brad and company accurately reanalyzed and recalibrated photographs of Pluto taken from the 1930s through the early 1950s. The really neat thing they found is that Pluto’s surface appearance changed a good amount during that time, indicating that frost deposits are migrating around the surface on a global scale due to seasonal and/or orbital distance changes. This has long been suspected, but Brad and his team could conclusively prove it because the parts of Pluto we could see in the early 1930s and early 1950s were identical – something that hasn’t occurred since. Their analysis of the old data using modern techniques made it possible to detect what astronomers of the mid-20th century had missed, and therefore allowed Shaffer’s team to rule out the competing theory – that Pluto’s changing photometric properties were just due to our seeing Pluto from differing angles over the decades. This result also confirms the prediction that global atmospheric change is important on Pluto. Indeed, this may even portend other kinds of changes (like day-to-day or day/night frost migration) will be discovered when New Horizons makes detailed surface maps as it approaches Pluto in 2015.

The other scientific result is about the planet’s largest moon, Charon. Submitted for publication by New Horizons co-investigator Mike Summers of George Mason University and three co-workers (myself included), the result is based on new computer models, rather than new data. These models show that some of Pluto’s escaping atmosphere is captured by Charon’s gravity, creating a tenuous atmosphere around Charon which – if confirmed by New Horizons – can be used to help diagnose the escape rate from Pluto.

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A schematic diagram showing potential flow patterns in Pluto’s escaping atmosphere.
Notice the bunching up around Charon, which will cause Charon to accrete an
atmosphere from Pluto.
(Credit: Mike Summers, George Mason University)


As I close, I want to tell you that the New Horizons project is “Twittering.” If you don’t know about Twitter, go to www.Twitter.com or look up Twitter on Wikipedia; it’s a micro-blogging service. Most weeks we will post a one-sentence update on what New Horizons is doing or where it is, or write something else interesting about the project. To get these updates, check out www.twitter.com/NewHorizons2015 from time to time, or create your own Twitter account and check the box to follow “NewHorizons2015” so you get updates whenever we post them. Pretty sweet –especially if my posts and the other occasional news items on the New Horizons Web page aren’t enough for you!

Well, that catches you up with where New Horizons is and what the spacecraft and project team have been doing. I’ll be back with more news in September. In the meantime, keep on exploring, just like we do.

- Alan Stern

Source: NASA/JHUPL - New Horizons
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