The Flickr Pioneerg Image Generatr

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This page simply reformats the Flickr public Atom feed for purposes of finding inspiration through random exploration. These images are not being copied or stored in any way by this website, nor are any links to them or any metadata about them. All images are © their owners unless otherwise specified.

This site is a busybee project and is supported by the generosity of viewers like you.

pio11_v_bw_o_n (76-H-430, 76-HC-600) by Mike Acs

© Mike Acs, all rights reserved.

pio11_v_bw_o_n (76-H-430, 76-HC-600)

“This enlargement of a Pioneer 11 picture covers part of Jupiter’s north temperature zone, and its north polar region. It shows the breakup of the regular banded structure of Jupiter’s clouds as one goes north toward the pole. The alternating, planet-girdling orange belts and grey-white zones, the most prominent features on the planet, first appear to break down into swirling scalloped and oval structures, and farther north to disappear completely. The northernmost part of the picture shows areas within 70 of the North Pole. According to Dr. Andrew Ingersoll, California Institute of Technology, these polar regions contain what appears to be an array of unorganized hurricane like convective storms. Many of these storms are circular, and some are several hundred miles across. Since Jupiter’s polar regions cannot be seen from Earth, this picture shows many features never seen before, and far the greatest array of details ever seen on the giant planet. Pioneer 11 flew within 42,000 km (26,000 mi) of Jupiter. This view was taken in blue light from 600,000 km (373,000 mi). The Pioneer Project is managed by NASA’s Ames Research Center, Mountain View, CA. and the Pioneer spacecraft were built by TRW Systems, Redondo Beach, Ca. The Jovian polar storms may be similar to Earth’s fast-spinning tropical hurricanes in that they are of similar size, and like hurricane may well be “heat pumps”, powered by the latent heat of condensation of water vapor and ammonia vapor. Sharply defined spiral features and scallops, most of them at the boundaries of high-latitude belt and zone regions are believed to result from the wind shears between adjacent, counterflowing jet streams produced in the belts and zones. Many of the jet streams producing these spiral features have speeds relative to the planet of 150 mph each, in opposite directions. This means 300 mph winds at [three words illegible]. Scientists believe that understanding of Jupiter’s Meteorology will lead to better understanding of weather on Earth. Jupiter is a liquid planet and hence has no solid surface, nor any “oceans”, only a gradual transition going down from atmosphere gat to liquid.”

The above is exactly how it’s written on the verso.

Compare/contrast:

bjj.mmedia.is/planet_rend/jup_north.jpg
Credit: Björn Jónsson's website (lots of really cool stuff there)

Finally:

"Figure 9-15. Image D8. Range 1,079,000 km (671,000 mi.), 13 1/2 hours after periapsis."

And:

"The series of images Figures 9-15 through 9-20 shows Jupiter receding as Pioneer 11 leaves the giant planet and rises high above the ecliptic plane on its way to Saturn. Due to an anomaly which affected the rate at which the telescope swept across the planet the command sequence to obtain these pictures had to be changed day by day. Nevertheless all were obtained without any being lost, despite the fact that there was no time to verify the command sequence by computer simulations in advance."

Both above from/at:

history.nasa.gov/SP-349/ch9.htm

Specifically:

history.nasa.gov/SP-349/p176.jpg

pio11_v_bw_v_n (AC71-8745, attached data sheet) by Mike Acs

© Mike Acs, all rights reserved.

pio11_v_bw_v_n (AC71-8745, attached data sheet)

pio11_v_bw_o_n (AC71-8745) by Mike Acs

© Mike Acs, all rights reserved.

pio11_v_bw_o_n (AC71-8745)

“In this picture the Pioneer 11 spacecraft is entering the thermal-vacuum chamber at TRW Space Systems Division in Redondo Beach, Ca.

The dish antenna focuses the 8-watt radio on the Earth almost one billion miles away. The spacecraft weighed at launch 570 lbs. This included 65 lbs. of scientific instruments. Pioneer 11 carries 11 onboard scientific instruments.

The Pioneer 11 spacecraft will make its closest approach to Saturn on September 1, and one of its moons, Titan on September 2.

The Pioneer Saturn project is managed by NASA’s Ames Research Center, Mountain View, Ca. The spacecraft was built by TRW.”

Awkwardly written, oddly only referencing the Saturn approach, with no mention of the year for that. But by golly it’ll be in ‘some’ September.
At least it indirectly brought attention to the puny power of the radio, the mind-boggling distance it had to transmit with that power, and the remarkably light weight of the spacecraft.

pio11_v_bw_v_n (AC71-8745) by Mike Acs

© Mike Acs, all rights reserved.

pio11_v_bw_v_n (AC71-8745)

pio11_v_bw_o_n (AC74-9213.1-B, AC74-9213) by Mike Acs

© Mike Acs, all rights reserved.

pio11_v_bw_o_n (AC74-9213.1-B, AC74-9213)

“This view, looking northward toward the equator, is the closest picture of Jupiter’s Great Red Spot taken by Pioneer 11. (Distance is 545,000 km or 338,000 mi).
More details of the Great Red Spot (which is large enough to swallow three Earths) and its surrounding region are visible here than have ever been seen before. The picture was taken in red and blue light and color.
Details of the flow, already known to exist, of the white cloud streams north of the Spot [flow] from right to left in the picture, and flow from left to right in the strip of clouds south of the Spot is clearly visible. The triangular regions on either side of the Spot appear to be areas where these two streams converge to flow side-by-side in opposite directions.
Details visible within the Spot (especially in the blue light picture) seem to show counterclockwise spiral there. Theory suggests that the Spot rotates counterclockwise due to the flow in the opposite directions of cloud streams north and south of it.
There also appears to be a narrow jet stream of brown material flowing southwestward above and to the left of the Spot. Strung out along the boundary between the white South Tropical zone, containing the Spot, and the brown belt north of it, is a series of small, white cloud puffs. (Puffs are only relatively small, typically about the size of Ohio). The puffs may be an example of flow instability between the zone and belt, where cloud currents are fastest relative to the planet.
The white oval below the right end of the Great Red Spot is one of three white ovals which are usually 120° apart around Jupiter, and have been known for 30 years. The oval’s position relative to the Red Spot changes with time due to a different rate of flow of the cloud current which contains it. New details of the white oval in this picture, such as the circular “eye” in its center, strongly suggest rotational motion.
Between the Red Spot and the white oval is a stream of brownish cloud material. Turbulance extending out to the right of the Spot seems to show (especially in the red light view) a large wake created by this atmosphere stream. This cloud stream appears to be one of the first examples seen of transfer of mass between the belts and zones, something predicted by theories on Jovian meteorology.
Pioneer 11, which took the picture, flew past Jupiter last December. The Pioneer Project is managed by NASA’s Ames Research Center, Mountain View, Ca. The spacecraft were built by TRW Systems.
Scientists believe that understanding of Jupiter’s Meteorology, and of other planets, will be of major importance in the understanding of weather on Earth.”

Also, the image (in color) and associated caption, on page 20:

“One of the best Pioneer images of Jupiter was obtained at a range of 545000 kilometers by Pioneer 11. Structure withing the Great Red Spot and the surrounding belts and zones can be seen. There was less turbulent cloud activity around the Spot at the times of the Pioneer flybys then was seen five years later by the Voyager cameras.”

At:

ntrs.nasa.gov/citations/19820018276

Finally:

From “NASA SP-446/PIONEER: FIRST TO JUPITER, SATURN, AND BEYOND”, pages 169 & 170 where the orthographic(?) projection of the image is shown as; (a) color composite, (b) blue channel image, and (c) red channel image, with the following accompanying text:

“For planetary astronomers, this image of the Great Red Spot of Jupiter was one of Pioneer 11’s most exciting results. From Pioneer 10, the highest-resolution image of the spot had been degraded by radiation problems, but Pioneer 11 obtained this unique image (Figure 9-11a). The area covered by the image on the planet is shown in the line drawing insert (d) on this page.

The image, obtained 545,000 km (339,000 miles) above the cloud tops, contains more than 4,000 individual pixels (see chapter 7) of measurable data in the red area of the spot a wealth of detailed markings since each pixel represents an area of approximately 237 km (147 miles) square. Scientists will be able to compare this image with those obtained by other spacecraft in later years to ascertain how the structure of the Spot changes with time.

Planetary scientists have derived new interpretations of the Great Red Spot from this image. Despite the relatively high resolution obtained, there is much less fine structure visible in the spot than in comparable areas at other latitudes (e.g., in Figure 9-12 and 914). The Great Red Spot appears to lie in the most quiescent zone of Jupiter, which may contribute to its stability.

The blue image has little internal detail (Figure 9-11b), the main feature being the dark border on the periphery of the spot. A break appears in the border in the northeast portion of the spot, where some of the red material appears to intermix with the South Tropical Zone.

The red image reveals much internal detail (Figure 9-11c), perhaps the most significant being two circular outlines that cross over near the center of the spot. This same feature also appeared in the Pioneer 10 images. This image does not show clear evidence of motions within the spot. The image does not show direct evidence of flow lines from any single region inside the spot, which could he interpreted as a source or a sink of red material.”

From/at:

atmos.nmsu.edu/data_and_services/atmospheres_data/SATURN/...

pio11_v_bw_o_n (ca. 1973, verso hand-annotated 525-e-4) by Mike Acs

© Mike Acs, all rights reserved.

pio11_v_bw_o_n (ca. 1973, verso hand-annotated 525-e-4)

Based solely on the similar 'look’ of Figure 6-22 at the following link, along with its associated text, which might even refer to this photo, this might be an image of Jupiter taken by Pioneer 11’s infrared radiometer. Or maybe it’s just a negative photo, intentional or otherwise. ¯\_(ツ)_/¯

~8” x 10.5”. From the estate of Eric Burgess.

The aforementioned text:

“In spite of the loss of some of the data covering the northern hemisphere of Jupiter when radiation affected the instrument, the infrared radiometer carried by Pioneer 11 provided two infrared spinscan images of the planet. A complete image was centered at 41° S and a partial image was centered at 52° N latitude on Jupiter. The ratio of total thermal energy to absorbed solar energy was revised to 1.9 ± 0.2 compared with previous estimates of 2.5 ± 0.5. The fact that both Pioneer 10 and Pioneer 11 data yield this result adds confidence in the new value.

Thus, Jupiter does not appear to be emitting as much internal heat as was once thought; about 24 percent less than had been assumed from Earth-based observations.

Jupiter's ionosphere rises 4000 km (2500 mi.) above the visible surface. It is ten times as thick and five times as hot as was predicted. Also, the ionosphere has at least five sharply defined layers of different density, similar to Earth's ionospheric layers that permit long range radio communication around Earth by returning certain radio waves to the ground.

The determination that Jupiter has a warm, extended, hydrogen rich atmosphere has important implications for further exploration of the giant planet.

Prior to measurements by the two Pioneers, it was generally considered that the heating of an entry probe into Jupiter's atmosphere would be greater than could be overcome by present-day technology. Now the new determinations of the Jovian atmosphere suggest that a probe can be made to survive entry into the Jovian atmosphere and measure directly its characteristics and constituents.

Enough has been confirmed or found out about Jupiter by the Pioneers to encourage further exploration. These two spacecraft have also demonstrated that such exploration is quite within the capabilities of present space technology which offers the opportunity now to sample directly what may be primordial material of the Solar System; thus, dipping back four and a half billion years in time.”

At:

history.nasa.gov/SP-349/ch6.htm

Specifically, Figure 6-22:

history.nasa.gov/SP-349/p121b.jpg

The truth may lie herein:

authors.library.caltech.edu/35833/
Credit: CaltechAUTHORS website

piofam_v_c_o_TPMBK (AC82-0178) by Mike Acs

© Mike Acs, all rights reserved.

piofam_v_c_o_TPMBK (AC82-0178)

“Pioneer Spacecraft Composite
"The Pioneer Family" Probes 6-9, 10, 11 and Venus Orbiter and Multiprobe or Bus (12-13)”

Also:

“The Pioneer Family (artistic images). Starting on the left, the first is the Pioneer 6, 7, 8,and 9 spacecraft. Next is the Pioneer 10 and 11 spacecraft. Next is the Pioneer Venus Orbiter (Pioneer 12) spacecraft. In the lower right corner is the Pioneer Venus Multiprobe (Pioneer 13) spacecraft.”

At:

www.nasa.gov/centers/ames/missions/archive/pioneer.html

Absolutely beautiful work by Michael Fornalski.
Right?! Who knew (him)??? Did you??? I didn’t!!!

commons.wikimedia.org/wiki/File:Pioneer_program.gif
Credit: Wikimedia Commons

archive.org/details/AILS-AC82-0178
Credit: the wonderful Internet Archives website

YES, another huge WIN…with a different twist! In comment (ca. April 2021) to a video posted by Scott Manley, entitled “Why NASA’s First Spaceflight Isn’t What Most People Think”, the following is Mr. Fornalski’s exact quote, specifically pertaining to this image, which is contained within the video:

“Another interesting trip in space history. Especially since you used an illustration I created for NASA-Ames way back in the 80’s, of the Pioneer spacecraft family. As I recall, it was for Program Director Richard Fimmel, who wanted a family picture image to use when he went out in public to give presentations on the Pioneer program at Ames. He had all the individual spacecraft art from other illustrators, he just wanted a group shot, so I repainted them as a composite. Fun project, as he gave me a tour around the building at Ames and there is just so much cool stuff there.”

At:

www.youtube.com/watch?v=Iao41k81q90
Credit: Scott Manley/YouTube

OUTSTANDING.

pio11_v_c_o_TPMBK (AC74-9041) by Mike Acs

© Mike Acs, all rights reserved.

pio11_v_c_o_TPMBK (AC74-9041)

“PIONEER 11 COURSE TOWARD INTERSTELLAR SPACE”

Probably the most beautiful, creative & striking version 😉 out of hundreds, if not thousands, depicting Pioneer 11’s historic mission and path to infinity…and beyond.

It being an Ames Research Center image, from 1974, of a Pioneer-Jupiter spacecraft, with dynamic ‘space’, I gotta go with Rick Guidice.

Despite the rendering, I'm pretty sure the spacecraft didn't fly between Saturn and its rings. Note also the outline of an unpainted deflection arrow at/behind "SPACE".

“INTERSTELLER”, UGH.

pio11_v_c_v_TPMBK (AC79-9103, attached data sheet) by Mike Acs

© Mike Acs, all rights reserved.

pio11_v_c_v_TPMBK (AC79-9103, attached data sheet)

pio11_v_c_o_TPMBK (AC79-9103) by Mike Acs

© Mike Acs, all rights reserved.

pio11_v_c_o_TPMBK (AC79-9103)

“Color image of Saturn and its rings taken by the Pioneer 11 spacecraft at a range of 5,464,000 kilometers (3,395,170 miles) presents many new features of the planet. For example, the Encke Division in the outer ring of the rings is clearly resolved where previously it was blended with the Cassini Division between the two major rings. The belted structure of the planet is also beginning to emerge. A small dark spot at about 5 o'clock is due to a small bit of incorrect data which can be corrected on future reproductions. A small notch at the edge of the planet about 11 o'clock could either be a small bit of missing data or the shadow of a moon. The image was made on Monday, August 27, and has been processed by a team of experimenters at the University of Arizona.”

pio11_v_bw_o_n (AC79-9111.4, poss. AC79-9111.5) by Mike Acs

© Mike Acs, all rights reserved.

pio11_v_bw_o_n (AC79-9111.4, poss. AC79-9111.5)

This Pioneer 11 photograph of Saturn’s rings, supposedly taken on August 31, 1979, at a distance of 943,000 km (585,950 miles) from the planet, revealed amazing detail (for that time). Although now crude & primitive, this historic photograph revealed a new feature in the Cassini Division (commonly referred to as the ‘Cassini Gap’ previously), new features in the A-Ring, the discovery of the F-Ring, and a new moon, then designated 1979-S1. Although some uncertainty exists, the moon was likely/possibly Epimetheus, named so in 1983, following higher resolution imaging by the Voyager 1 spacecraft, along with more refined orbital calculations. However, caveat to the above is a reference to Epimetheus (at an ‘official’ NASA website mind you) as 1980-S3, so call it whatever you want. Tethys is to the upper left.

As there appears to be no stand-alone NASA or JPL listing of this/these images, the above is best effort at compiling from the content available at the following:

The exact images, oriented horizontally, on page 123:

atmos.nmsu.edu/data_and_services/atmospheres_data/SATURN/...

And:

www.nasa.gov/image-feature/45-years-ago-pioneer-11-launch...

Specifically, whereas within the URL the photo identification of 'AC79-9111.5' is embedded:

www.nasa.gov/sites/default/files/thumbnails/image/ac79-91...

Finally:

www.fossilhunters.xyz/saturn-ring-system/encounters-with-...
Credit: Dennis Larson/"Fossil Hunters" blogsite

en.wikipedia.org/wiki/Epimetheus_(moon)
Credit: Wikipedia

solarsystem.nasa.gov/moons/saturn-moons/epimetheus/in-dep...

pio11_v_c_o_TPMBK (AC74-9006.4) by Mike Acs

© Mike Acs, all rights reserved.

pio11_v_c_o_TPMBK (AC74-9006.4)

“Artist’s conception showing Pioneer 11 as it will look passing Saturn in September 1979. Pioneer’s passage of the ringed planet will be the first flight to Saturn, which is 887 million miles from the Sun. Tentative plans call for Pioneer 11 to fly through the space between the inner ring and the planet’s cloud tops, and then to come close to Saturn’s large moon, Titan. Titan’s environment is considered favorable for living organisms. After passing Saturn and photographing and measuring the planet, its rings and moons, the spacecraft will leave the solar system altogether. Pioneer 11 flew past Jupiter in December 1974.”

See also:

www.nasa.gov/sites/default/files/thumbnails/image/ac74-90...

www.nasa.gov/image-feature/45-years-ago-pioneer-11-launch...

An interesting inverted variant of this serves as the cover art of the NASA/Ames Research Center publication, "PIONEER SATURN ENCOUNTER":

www.gutenberg.org/files/55695/55695-h/55695-h.htm
Credit: Project Gutenberg website
Which looks to be well worth exploring further...FREE eBooks...outstanding!

Interesting background information on Mr. Guidice:

www.sciencefriday.com/articles/this-70s-artist-painted-ou...

www.numulosgatos.org/exhibitions-2/2015/9/17/rick-guidice...

pio10-11_v_bw_o_n (Ames Research Center photo, hand-annotated A73-4887.1) by Mike Acs

© Mike Acs, all rights reserved.

pio10-11_v_bw_o_n (Ames Research Center photo, hand-annotated A73-4887.1)

Striking & fanciful artist's concept of Pioneer 10 and/or 11 transiting the Jovian system during its historic flyby mission.

I assume that’s the sun. If so, it’s kinda big from that far out. Uh oh...maybe it’s going nova!

pio11_v_bw_o_n (Ames Research Center photo, hand-annotated A73-9013) by Mike Acs

© Mike Acs, all rights reserved.

pio11_v_bw_o_n (Ames Research Center photo, hand-annotated A73-9013)

Pioneer G/11 is prepared for encapsulation at the Kennedy Space Center. In one of the two Spacecraft Assembly and Encapsulation Facilities?

Content of "SP-349/396: PIONEER ODYSSEY" seems to indicate SAEF-1/Building AO:

history.nasa.gov/SP-349/ch5.htm

history.nasa.gov/SP-349/p64a.jpg

See also:

www.nasa.gov/centers/ames/images/content/72422main_A73-90...

pio10-11_v_bw_o_n (72-H-138, 72-HC-108, AC72-1351 eq) by Mike Acs

© Mike Acs, all rights reserved.

pio10-11_v_bw_o_n (72-H-138, 72-HC-108, AC72-1351 eq)

Excellent artist's concept of the Pioneer spacecraft over the Jovian cloud tops.

In color:

images.nasa.gov/details-ARC-1969-AC72-1351

Obviously, one or the other is reversed. Which one? We/I may never know.

piofg_v_c_o_AKP (prob TRW photographic services photo no. 67881-69) by Mike Acs

© Mike Acs, all rights reserved.

piofg_v_c_o_AKP (prob TRW photographic services photo no. 67881-69)

Before Juno, New Horizons (when it zoomed by), before Galileo...EVEN BEFORE Voyager, there were Pioneers...10 & 11...first to Jupiter.

Beautiful EARLY (1969?) depiction by resident TRW artist/Art Director Frank Warren, of the intrepid little spacecraft at its destination.

Until 17 February 1998, it was the most distant spacecraft from the Sun. On that day, at the mind-boggling distance of 69.419 AU, Voyager 1 overtook it...so Voyager is seriously hauling ass...it was launched FIVE years after Pioneer 10. Voyager 1 is in fact moving away from the Sun at over 1 AU/year faster than Pioneer 10.

Last contact with Pioneer 10 was in 2003.

Interesting reading, especially WRT the primary mission of the spacecraft. Really???

airandspace.si.edu/multimedia-gallery/nasm-nasm-7b24156jpg

Additional informative reading:

www.nasa.gov/topics/history/features/Pioneer_10_40th_Anni...

Last, but NOT least, Frank Warren...remembered:

www.independent.com/obits/2017/09/18/frank-warren/
Credit: Santa Barbara Independent website

LDKPSK/pio11_v_c_o_TPMBK (AC74-9007) by Mike Acs

© Mike Acs, all rights reserved.

LDKPSK/pio11_v_c_o_TPMBK (AC74-9007)

“Saturn from Titan: by Ludek Pesek”, faintly visible in the lower right border.

“Artist Ludek Pesek's depiction of the planet Saturn as it would appear to astronauts landing on Titan, largest satellite of Saturn. Pioneer 11, after a rendezvous with Jupiter in December, 1974, will arrive at Saturn in September 1979.”

Featured as the cover of the September 1976 issue of ‘Space World’ magazine.

Amazing & memorable work:

www.ludekpesek.ch/

piofg_v_c_o_AKP (TRW photographic services photo no. 78616-70-5) by Mike Acs

© Mike Acs, all rights reserved.

piofg_v_c_o_AKP (TRW photographic services photo no. 78616-70-5)

Technicians prepare the Pioneer F spacecraft, OR a Pioneer F/G thermal model(?) - for testing in the Space Simulation Chamber at TRW Systems, Redondo Beach, California, ca. 1970(?)

Good stuff also at:

www.spaceflightinsider.com/space-flight-history/our-space...

www.spaceflightinsider.com/space-flight-history/spaceflig...

Specifically:

www.spaceflightinsider.com/wp-content/uploads/2014/06/The...

And compare to Pioneer H (aka Pioneer 12), if it would've flown, on display at the NASM:

www.spaceflightinsider.com/wp-content/uploads/2015/06/Pio...

Credit: Space Flight Insider website & Creative Commons

pio11_v_c_o_TPMBK (29 Nov 79, AC79-9107.2, AC79-9107.3?, 79-HC-551 eq) by Mike Acs

© Mike Acs, all rights reserved.

pio11_v_c_o_TPMBK (29 Nov 79, AC79-9107.2, AC79-9107.3?, 79-HC-551 eq)

“This image from Pioneer 11 shows Saturn and its moon Titan. The irregularities in ring silhouette and shadow are due to technical anomalies in the preliminary data later corrected. At the time this image was taken, Pioneer was 2,846,000 km (1,768,422 miles) from Saturn.”

www.nasa.gov/sites/default/files/739460main_ac79-9107.3.jpg

solarsystem.nasa.gov/resources/722/pioneer-11-at-saturn/

And/or:

“Shown here is the best view yet available of Saturn and its rings, returned by the Pioneer spacecraft during its encounter with the ringed planet...

The view was taken by Pioneer Saturn from a distance of 2,500,000 kilometers (1,500,000 miles) on August 29, 1979, 58 hours before closest approach. Resolution is better than Earth-based quality....”