|
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Titania's Trenches
| Title |
Titania's Trenches |
| Explanation |
British astronomer Sir William Herschel [ http://star.arm.ac.uk/history/herschel.html ] discovered Titania and Oberon in January of 1787. He wasn't reading Shakespeare's [ http://the-tech.mit.edu/Shakespeare/works.html ]"A Midsummer Night's Dream" though, he was making the first telescopic observations of moons of the planet Uranus [ http://seds.lpl.arizona.edu/nineplanets/nineplanets/uranus.html ] (a planet which he himself discovered in 1781 [ http://www-groups.dcs.st-and.ac.uk/~history/ HistTopics/Neptune_and_Pluto.html ]). In January of 1986, nearly 200 years later, NASA's robot explorer Voyager 2 became the only spacecraft to visit the remote Uranian [ http://antwrp.gsfc.nasa.gov/apod/ap990531.html ] system [ http://antwrp.gsfc.nasa.gov/apod/ap971103.html ]. Above is Voyager's highest resolution picture of Titania [ http://photojournal.jpl.nasa.gov/cgi-bin/ PIAGenCatalogPage.pl?PIA00039 ], Uranus' largest moon. The picture is a composite of two images recorded from a distance of 229,000 miles. The icy, rocky world [ http://antwrp.gsfc.nasa.gov/apod/ap960304.html ] is seen to be covered with impact craters. A prominent system of fault valleys, some nearly 1,000 miles long, is visible as trench-like features near the terminator (shadow line). Deposits of highly reflective material which may represent frost can be seen along the sun-facing valley walls. The large impact crater near the top, known as Gertrude [ http://wwwflag.wr.usgs.gov/USGSFlag/Space/nomen/uranus/titacrat.html ], is about 180 miles across. At the bottom the 60 mile wide fault valley, Belmont Chasma [ http://wwwflag.wr.usgs.gov/USGSFlag/Space/nomen/uranus/titachas.html ], cuts into crater Ursula. Titania itself [ http://wwwflag.wr.usgs.gov/USGSFlag/Space/wall/titania.html ] is 1,000 miles in diameter. |
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Verona Rupes: Tallest Known
…
| Title |
Verona Rupes: Tallest Known Cliff in the Solar System |
| Explanation |
Could you survive a jump off the tallest cliff in the Solar System? Quite possibly. Verona Rupes [ http://en.wikipedia.org/wiki/Verona_Rupes ] on Uranus [ http://www.nineplanets.org/uranus.html ]' moon Miranda [ http://www.nineplanets.org/miranda.html ] is estimated to be 20 kilometers deep -- ten times the depth of the Earth's Grand Canyon [ http://www.nps.gov/grca/ ]. Given Miranda [ http://en.wikipedia.org/wiki/Miranda_%28moon%29 ]'s low gravity, it would take about 12 minutes for a thrill-seeking adventurer [ http://video.google.com/videoplay?docid=2090669779765584576 ] to fall from the top, reaching the bottom at the speed of a racecar -- about 200 kilometers per hour. Even so, the fall might be survivable given proper airbag [ http://www.howstuffworks.com/airbag.htm ] protection. The above image [ http://photojournal.jpl.nasa.gov/catalog/PIA00044 ] of Verona Rupes was captured by the passing Voyager [ http://antwrp.gsfc.nasa.gov/apod/ap020831.html ] 2 robotic spacecraft in 1986. How the giant cliff was created remains unknown, but is possibly related to a large impact [ http://antwrp.gsfc.nasa.gov/apod/ap050308.html ] or tectonic [ http://en.wikipedia.org/wiki/Extensional_tectonics ] surface motion. |
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Uranus: The Tilted Planet
| Title |
Uranus: The Tilted Planet |
| Explanation |
Uranus is the third largest planet in our Solar System [ http://www.nineplanets.org/overview.html ] after Jupiter [ http://antwrp.gsfc.nasa.gov/apod/jupiter.html ] and Saturn [ http://antwrp.gsfc.nasa.gov/apod/ap010826.html http://www.solarviews.com/eng/saturn.htm ]. Uranus [ http://www.nineplanets.org/uranus.html ] is composed mostly of rock and ices, but with a thick hydrogen [ http://chemlab.pc.maricopa.edu/periodic/h.html ] and helium [ http://antwrp.gsfc.nasa.gov/apod/ap010120.html ] atmosphere. The blue hue of Uranus' atmosphere arises from the small amount of methane [ http://scifun.chem.wisc.edu/chemweek/methane/methane.html ] which preferentially absorbs red light. This picture [ http://photojournal.jpl.nasa.gov/cgi-bin/PIAGenCatalogPage.pl?PIA01360 ] was snapped by the Voyager 2 spacecraft [ http://nssdc.gsfc.nasa.gov/planetary/voyager.html ] in 1986 - the only spacecraft ever to visit Uranus. Uranus [ http://antwrp.gsfc.nasa.gov/apod/uranus.html ] has many moons [ http://antwrp.gsfc.nasa.gov/apod/ap990531.html ] and a ring system [ http://antwrp.gsfc.nasa.gov/apod/ap971126.html ]. Uranus, like Venus [ http://antwrp.gsfc.nasa.gov/apod/venus.html ], has a rotation axis that is greatly tilted and sometimes points near the Sun. It remains an astronomical mystery why Uranus' axis [ http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=1991LPIP...22...59S ] is so tilted. Uranus and Neptune [ http://antwrp.gsfc.nasa.gov/apod/neptune.html ] are quite similar: Uranus is slightly larger but less massive. |
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Jupiter's Rings
| Title |
Jupiter's Rings |
| Explanation |
Astronomers using NASA's Voyager [ http://nssdc.gsfc.nasa.gov/planetary/voyager.html ] spacecraft to search for a ring system around Jupiter discovered these faint rings in 1979. Unlike Saturn's bright rings which are composed of chunks of rock and ice, Jupiter's rings [ http://ringside.arc.nasa.gov/www/jupiter/jupiter.html ] appear to consist of fine particles of dust. One possibility is that the dust is produced by impacts with Jupiter's inner moons. This false color image has been computer enhanced. The gas giant planets, Jupiter, Saturn, Uranus, and Neptune are all known to have rings. For more information about planetary ring systems see the Planetary Rings Node [ http://ringside.arc.nasa.gov/ ]. Tomorrow's picture: A Volcanic Moon |
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Neptune: Big Blue Giant
| Title |
Neptune: Big Blue Giant |
| Explanation |
This picture was taken by the Voyager 2 [ http://nssdc.gsfc.nasa.gov/planetary/voyager.html ] spacecraft in 1986 - the only spacecraft ever to visit Neptune. Neptune [ http://seds.lpl.arizona.edu/nineplanets/nineplanets/neptune.html ] will be the farthest planet from the Sun [ http://antwrp.gsfc.nasa.gov/apod/ap950813.html ] until 1999, when the elliptical orbit of Pluto will cause it to once again resume this status. Neptune [ http://www.c3.lanl.gov/~cjhamil/SolarSystem/neptune.html ], like Uranus [ http://antwrp.gsfc.nasa.gov/apod/ap950816.html ], is composed mostly of liquid water, methane and ammonia, is surrounded by a thick gas atmosphere of mostly hydrogen and helium, and has many moons and rings. Neptune [ http://nssdc.gsfc.nasa.gov/photo_gallery/photogallery-neptune.html ]'s moon Triton [ http://antwrp.gsfc.nasa.gov/apod/ap950805.html ] is unlike any other and has active volcanoes. The nature of Triton [ http://seds.lpl.arizona.edu/nineplanets/nineplanets/triton.html ]'s unusual orbit around Neptune is the focus of much discussion and speculation. Tomorrow's picture: Pluto: The Frozen Planet |
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Uranus' Moon Miranda
| Title |
Uranus' Moon Miranda |
| Explanation |
NASA's robot spacecraft Voyager 2 passed the planet Uranus [ http://antwrp.gsfc.nasa.gov/apod/ap950816.html ] and its moons in 1986. While the cloud tops of Uranus [ http://seds.lpl.arizona.edu/nineplanets/nineplanets/uranus.html ] proved to be rather featureless, the surface of Miranda [ http://seds.lpl.arizona.edu/nineplanets/nineplanets/miranda.html ], the innermost of Uranus [ http://www.c3.lanl.gov/~cjhamil/SolarSystem/uranus.html ]' large moons, showed several interesting features. Voyager 2 passed closer to Miranda [ http://www.c3.lanl.gov/~cjhamil/SolarSystem/miranda.html ] than to any Solar System [ http://antwrp.gsfc.nasa.gov/apod/ap950819.html ] body and hence photographed it with the clearest resolution. Miranda's heavily cratered terrain shows grooves like Jupiter [ http://antwrp.gsfc.nasa.gov/apod/ap951208.html ]'s moon Ganymede [ http://antwrp.gsfc.nasa.gov/apod/ap950904.html ] and several valleys and cliffs. Miranda is made of a roughly equal mix of ice and rock. Miranda was discovered by Gerard Kuiper in 1948. |
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Uranus' Moon Ariel: Valley W
…
| Title |
Uranus' Moon Ariel: Valley World |
| Explanation |
What formed Ariel [ http://bang.lanl.gov/solarsys/ariel.htm ]'s valleys? This question presented itself when Voyager [ http://vraptor.jpl.nasa.gov/voyager/voyager.html ] 2 passed this satellite of Uranus [ http://antwrp.gsfc.nasa.gov/apod/ap950816.html ] in January 1986. Speculation [ http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1990Icar%2E%2E%2E87%2E%2E110T&db_key=AST ] includes that heating caused by the ancient tides of Uranus caused moonquakes and massive shifting of the moon's surface. In any event, a huge network of sunken valleys was found to cover this frozen moon, and some unknown material now coats the bottoms of many of these channels. Ariel [ http://seds.lpl.arizona.edu/nineplanets/nineplanets/ariel.html ] is the second closest to Uranus outside of Miranda [ http://antwrp.gsfc.nasa.gov/apod/ap951224.html ], and is composed of roughly half water ice and half rock. Ariel was discovered by William Lassell [ http://seds.lpl.arizona.edu/nineplanets/nineplanets/help.html#lassell ] in 1851. |
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Two Hours Before Neptune
| Title |
Two Hours Before Neptune |
| Explanation |
Two hours before closest approach to Neptune [ http://www.nineplanets.org/neptune.html ] in 1989, the Voyager 2 [ http://vraptor.jpl.nasa.gov/voyager/vgrfaqs.html ] robot spacecraft snapped this picture [ http://nssdc.gsfc.nasa.gov/photo_gallery/photogallery-neptune.html ]. Clearly visible for the first time were long light-colored cirrus [ http://www.bham.ac.uk/geography/met/clouds/h1.htm ]-type clouds floating high in Neptune's atmosphere [ http://nssdc.gsfc.nasa.gov/photo_gallery/caption/neptune_clouds.txt ]. Shadows of these clouds can even be seen on lower cloud decks. Most of Neptune's atmosphere [ http://antwrp.gsfc.nasa.gov/apod/ap960507.html ] is made of hydrogen [ http://chemlab.pc.maricopa.edu/periodic/h.html ] and helium [ http://chemlab.pc.maricopa.edu/periodic/He.html ], which is invisible. Neptune's blue color therefore comes from smaller amounts of atmospheric methane [ http://www.epa.gov/ghginfo/ ], which preferentially absorbs red light. Neptune [ http://pds.jpl.nasa.gov/planets/welcome/neptune.htm ] has the fastest winds in the Solar System [ http://www.nineplanets.org/overview.html ], with gusts reaching 2000 kilometers per hour. Speculation [ http://www.berkeley.edu/news/berkeleyan/1999/1006/diamonds.html ] holds that diamonds [ http://www.sdnhm.org/exhibits/diamonds/facts.html ] may be created in the dense hot conditions that exist under the clouds-tops of Uranus [ http://spacelink.msfc.nasa.gov/Instructional.Materials/Curriculum.Support/Space.Science/Our.Solar.System/Uranus/ ] and Neptune. |
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Uranus' Largest Moon: Titani
…
| Title |
Uranus' Largest Moon: Titania |
| Explanation |
Titania's tortured terrain is a mix of valleys and craters. NASA's interplanetary robot spacecraft Voyager [ http://spacelink.msfc.nasa.gov/NASA.Projects/Planetary.Probes/Voyager/Mission.Summary ] 2 passed this moon of Uranus [ http://antwrp.gsfc.nasa.gov/apod/ap950816.html ] in 1986 and took the above photograph. The photograph was then transmitted back to earth by radio [ http://www.science.uwaterloo.ca/physics/p13news/number_2/maxnew-2.html ]. The valleys of Titania [ http://bang.lanl.gov/solarsys/titania.htm ] resemble those on Ariel [ http://antwrp.gsfc.nasa.gov/apod/ap960303.html ] indicate that Titania underwent some unknown tumultuous resurfacing event in its distant past. Although Titania [ http://seds.lpl.arizona.edu/nineplanets/nineplanets/titania.html ] is Uranus' largest moon, it is still much smaller than Triton [ http://antwrp.gsfc.nasa.gov/apod/ap950805.html ] - the largest moon of Uranus' sister planet Neptune [ http://antwrp.gsfc.nasa.gov/apod/ap950817.html ]. Titania is essentially a large dirty iceball that orbits Uranus - it is composed of about half water-ice and half rock. Titania was discovered by William Hershel [ http://www.dsi.unimi.it/Users/Students/amoroso/sun/fortunes/life-e.html ] in 1787. |
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Uranus's Moon Oberon: Impact
…
| Title |
Uranus's Moon Oberon: Impact World |
| Explanation |
Oberon is the most distant and second largest moon of Uranus. Discovered by William Herschel [ http://www.adventure.com/library/encyclopedia/space/herschls.html ] in 1787, the properties of the world remained relatively unknown until the robot spacecraft Voyager [ http://vraptor.jpl.nasa.gov/voyager/voyager.html ] 2 passed it during its flyby of Uranus [ http://antwrp.gsfc.nasa.gov/apod/ap950816.html ] in January 1986. Compared to Uranus' moons Ariel [ http://antwrp.gsfc.nasa.gov/apod/ap960303.html ], Titania [ http://antwrp.gsfc.nasa.gov/apod/ap960304.html ], and Miranda [ http://antwrp.gsfc.nasa.gov/apod/ap951224.html ], Oberon [ http://seds.lpl.arizona.edu/nineplanets/nineplanets/oberon.html ] is heavily cratered, and in this way resembles Umbriel [ http://antwrp.gsfc.nasa.gov/apod/ap960407.html ]. Like all of Uranus' large moons, Oberon [ http://bang.lanl.gov/solarsys/oberon.htm ] is composed of roughly half ice and half rock. Note that Oberon has at least one large mountain, visible on the limb at the lower left, that rises 6 km off the surface. |
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Uranus's Moon Umbriel: A Mys
…
| Title |
Uranus's Moon Umbriel: A Mysterious Dark World |
| Explanation |
Why is Umbriel so dark? This dark moon reflects only half the light of other Uranus' [ http://antwrp.gsfc.nasa.gov/apod/ap950816.html ] moons such as Ariel [ http://antwrp.gsfc.nasa.gov/apod/ap960303.html ]. And what is that bright ring at the top? Unfortunately, nobody yet knows. These questions presented themselves when Voyager [ http://vraptor.jpl.nasa.gov/voyager/voyager.html ] 2 passed this satellite of Uranus [ http://antwrp.gsfc.nasa.gov/apod/ap950816.html ] in January 1986. Voyager found an old surface with unusually large craters, and determined Umbriel [ http://seds.lpl.arizona.edu/nineplanets/nineplanets/umbriel.html ]'s composition to be about half ice and half rock. Umbriel [ http://bang.lanl.gov/solarsys/umbriel.htm ] is the fourth largest and third most distant of Uranus' five large moons. Umbriel was discovered in 1851 by William Lassell [ http://www.ast.cam.ac.uk/~naw96/lassell/lassell.htm ]. |
|
Ringed Planet Uranus
| Title |
Ringed Planet Uranus |
| Explanation |
Yes it does look like Saturn, but Saturn is only one of four [ http://antwrp.gsfc.nasa.gov/apod/ap020616.html ] giant [ http://antwrp.gsfc.nasa.gov/apod/ap020215.html ] ringed [ http://antwrp.gsfc.nasa.gov/apod/ap981020.html ] planets [ http://ringmaster.arc.nasa.gov/neptune/neptune.html ] in our Solar System. And while Saturn has the brightest rings, this system of rings and moons actually belongs to planet Uranus, imaged here [ http://www.eso.org/outreach/press-rel/pr-2002/ phot-31-02.html ] in near-infrared light by the Antu [ http://antwrp.gsfc.nasa.gov/apod/ap000707.html ] telescope at the ESO Paranal Observatory in Chile. Since gas giant Uranus' [ http://www.seds.org/nineplanets/nineplanets/uranus.html ] methane-laced atmosphere absorbs sunlight at near-infrared wavelengths the planet appears substantially darkened, improving the contrast between the otherwise relatively bright planet and the normally faint rings. In fact, the narrow Uranian rings [ http://ringmaster.arc.nasa.gov/uranus/ uranus.html ] are all but impossible to see in visible light with earthbound telescopes and were discovered [ http://tdc-www.harvard.edu/occultations/ uranus25/ ] only in 1977 as careful astronomers noticed the then unknown rings blocking light from background stars. The rings are thought to be younger than 100 million years and may be formed of debris from the collision of a small moon with a passing comet or asteroid-like object. With moons [ http://antwrp.gsfc.nasa.gov/apod/ap000930.html ] named for characters [ http://antwrp.gsfc.nasa.gov/apod/ap990227.html ] in Shakespeare's plays, the distant ringed world Uranus [ http://vraptor.jpl.nasa.gov/voyager/vgrur_fs.html ] was last visited in 1986 by the Voyager 2 spacecraft. |
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Solar System Portrait
| Title |
Solar System Portrait |
| Explanation |
On another Valentine's Day [ http://www.poets.org/poems/poems.cfm?prmID=1166 ] (February 14, 1990), cruising four billion miles from the Sun, the Voyager 1 [ http://antwrp.gsfc.nasa.gov/apod/ap031120.html ] spacecraft looked back to make this first ever family portrait [ http://photojournal.jpl.nasa.gov/cgi-bin/ PIAGenCatalogPage.pl?PIA00451 ] of our Solar System. The complete portrait is a 60 frame mosaic [ http://nssdc.gsfc.nasa.gov/photo_gallery/ photogallery-solarsystem.html ] made from a vantage point 32 degrees above the ecliptic plane [ http://antwrp.gsfc.nasa.gov/apod/ap001014.html ]. Voyager's wide angle camera frames sweep through the inner Solar System (far left) linking up with gas giant Neptune, at the time the Solar System's [ http://www.seds.org/nineplanets/nineplanets/overview.html ] outermost planet (scroll right). Positions [ http://nssdc.gsfc.nasa.gov/image/planetary/solar_system/ family_diagram.jpg ] for Venus, Earth [ http://www.seds.org/billa/psc/pbd.html ], Jupiter, Saturn, Uranus, and Neptune are indicated by the corresponding letters while the Sun is the bright spot near the center of the circle of frames. The inset frames [ http://antwrp.gsfc.nasa.gov/apod/ap980517.html ] for each of the planets are from Voyager's narrow field camera. Unseen in the portrait are Mercury [ http://www.psrd.hawaii.edu/Jan97/Mercury Unveiled.html ], too close to the Sun to be detected, and Mars, unfortunately hidden by sunlight scattered in the camera's optical system. Small, faint Pluto's [ http://antwrp.gsfc.nasa.gov/apod/ap011018.html ] position was not covered. |
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Irregular Moons Discovered A
…
| Title |
Irregular Moons Discovered Around Uranus |
| Explanation |
Where did these two irregular moons of Uranus [ http://www.seds.org/nineplanets/nineplanets/uranus.html ] originate? Last week two previously undiscovered moons [ http://www.cita.utoronto.ca/~gladman/utpress.html ] of the distant gas planet were confirmed [ http://cfa-www.harvard.edu/iauc/06700/06765.html ], the first in irregular orbits. All fifteen previously known moons [ http://www.seds.org/nineplanets/nineplanets/uramoons.html ] of Uranus [ http://bang.lanl.gov/solarsys/uranus.htm ] are 'regular', circling near the planet's equator. Most of these were discovered by the passing Voyager 2 spacecraft [ http://vraptor.jpl.nasa.gov/voyager/voyager.html ] in 1986. These newly discovered moons [ http://www.news.cornell.edu/science/Oct97/new_moons.hrs.html ] are thought to be odd-shaped and about 100 km across. They are considered irregular, though, because they orbit in odd directions and far from Uranus [ http://antwrp.gsfc.nasa.gov/apod/ap950816.html ]. If Uranus' irregular moons have the same origin as those orbiting Jupiter [ http://www.seds.org/nineplanets/nineplanets/jupiter.html ], Saturn [ http://pds.jpl.nasa.gov/planets/welcome/saturn.htm ], and Neptune [ http://spacelink.msfc.nasa.gov/Instructional.Materials/Curriculum.Materials/Sciences/Astronomy/Our.Solar.System/Neptune/ ], then they were probably caught from orbits around the Sun [ http://antwrp.gsfc.nasa.gov/apod/ap960518.html ]. Moons like this are discovered by their motion. One of these moons is shown above [ http://www.cita.utoronto.ca/~gladman/ ] as the circled point of light moving from left to right. (To stop the movie from repeating, click "stop" on most browsers.) |
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Hamlet of Oberon
| Title |
Hamlet of Oberon |
| Explanation |
What's in a name? [ http://the-tech.mit.edu/Shakespeare/Quotes/bart.RJ.html#22 ] Since 1919, the International Astronomical Union [ http://www.intastun.org ] has been charged with the task [ http://the-tech.mit.edu/Shakespeare/Quotes/bart.LoveLost.html#3 ] of establishing "conventional" nomenclature [ http://wwwflag.wr.usgs.gov/USGSFlag/Space/nomen/nomen.html ] for planets, satellites, and surface features. For the remote Uranian system [ http://antwrp.gsfc.nasa.gov/apod/ap971126.html ] of moons, namesakes from Shakespearean works [ http://the-tech.mit.edu/Shakespeare/works.html ] have been chosen. Thus Oberon [ http://antwrp.gsfc.nasa.gov/apod/ap960408.html ], king of the mid-summer night fairies, is also Uranus' most distant and second largest moon [ http://antwrp.gsfc.nasa.gov/apod/ap970111.html ]. Hamlet is the tragically dark, large and princely crater on its surface [ http://wwwflag.wr.usgs.gov/USGSFlag/Space/nomen/uranus/obercrat.html ] (right of center). The above image represents known surface features of Oberon [ http://wwwflag.wr.usgs.gov/USGSFlag/Space/wall/oberon.html ] and was constructed by the U.S. Geological Survey (USGS) based on data from NASA's robot explorer Voyager 2 [ http://vraptor.jpl.nasa.gov/voyager/voyager_fs.html ]. In 1986, Voyager 2 flew through the Uranian system [ http://vraptor.jpl.nasa.gov/voyager/vgrur_fs.html ] - so far it has been the only spacecraft to do so [ http://nssdc.gsfc.nasa.gov/imgcat/html/mission_page/ UR_Voyager_2_page1.html ]. |
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Miranda, Chevron, and Alonso
| Title |
Miranda, Chevron, and Alonso |
| Explanation |
Miranda [ http://www.seds.org/nineplanets/nineplanets/miranda.html ] is a bizarre world which surely had a tempest [ http://the-tech.mit.edu/Shakespeare/Comedy/tempest/thetempest.html ]uous past. The innermost of the larger Uranian [ http://pds.jpl.nasa.gov/planets/welcome/uranus.htm ] moons, Miranda is almost 300 miles in diameter and was discovered [ http://antwrp.gsfc.nasa.gov/apod/ap971103.html ] in 1948 by American planetary astronomer Gerard Kuiper [ http://sofia.arc.nasa.gov/KAO/home/kuiper_bio.html ]. Examined very closely by the Voyager 2 spacecraft [ http://vraptor.jpl.nasa.gov/voyager/voyager_fs.html ] in 1986, this dark and distant world turned out to be [ http://vraptor.jpl.nasa.gov/voyager/vgrur_fs.html ] quite a surprise [ http://www.pbm.com/~lindahl/music_and_dance.html ]. Miranda was found to display [ http://www.seds.org/nineplanets/nineplanets/pxuranus.html#Miranda ] a unique, bewildering variety of [ http://www.shakespeare.mcgill.ca/resources/ ] terrain leading some to suggest that it has been fractured up to 5 times during its evolution. Along with the famous "chevron" feature, the bright V-shaped area just above center, this composite of the highest resolution images of Miranda shows [ http://www.hawastsoc.org/solar/cap/uranus/vmiranda.htm ] wild juxtapositions of ridges and valleys, older cratered and younger smooth surfaces, and shadowy canyons perhaps 12 miles deep. The large crater (below center) is the 15 mile wide crater Alonso [ http://the-tech.mit.edu/Shakespeare/Comedy/tempest/ thetempest.dp.html ]. |
|
A Solar System Portrait
| Title |
A Solar System Portrait |
| Explanation |
As the Voyager 1 spacecraft [ http://vraptor.jpl.nasa.gov/voyager/vgrfaqs.html ] headed out of our Solar System [ http://antwrp.gsfc.nasa.gov/apod/ap980517.html ], it looked back and took a parting family portrait [ http://nssdc.gsfc.nasa.gov/photo_gallery/photogallery-solarsystem.html ] of the Sun [ http://www.seds.org/nineplanets/nineplanets/sol.html ] and planets. From beyond Pluto [ http://antwrp.gsfc.nasa.gov/apod/ap990213.html ], our Solar System looks like a bright star surrounded by faint dots. In the above picture [ http://photojournal.jpl.nasa.gov/cgi-bin/PIAGenCatalogPage.pl?PIA00451 ], the Sun is so bright it is blocked out for contrast. The innermost dots visible, labeled E and V for Earth [ http://antwrp.gsfc.nasa.gov/apod/ap990131.html ] and Venus [ http://www.nasm.edu/ceps/RPIF/VENUS/rpifvenus.html ], are particularly hard to discern. Gas giants Jupiter [ http://www.jpl.nasa.gov/galileo/Jovian.html ] (J) and Saturn [ http://www.seds.org/nineplanets/nineplanets/saturn.html ] (S) are much more noticeable. The outermost planets visible are Uranus [ http://www.hawastsoc.org/solar/eng/uranus.htm ] (U) and Neptune [ http://antwrp.gsfc.nasa.gov/apod/ap980221.html ] (N). Each planet is shown labeled and digitally enhanced in an inset image. Voyager 1 is only one of four human-made objects to leave our Solar System, the other three being Voyager 2, and Pioneer 10 and Pioneer 11. |
|
Uranus' Moon 18
| Title |
Uranus' Moon 18 |
| Explanation |
The discovery was there for the taking. An image of Uranus [ http://www.seds.org/nineplanets/nineplanets/uranus.html ] taken by Voyager [ http://nssdc.gsfc.nasa.gov/planetary/voyager.html ] 2 as it passed the giant planet 13 years ago apparently recorded a moon that had since gone unnoticed. The image on which Uranus' 18th moon was discovered was freely available [ http://www-pdsimage.JPL.NASA.GOV/PDS/public/jukebox.html ] from NASA. Erich Karkoschka (U. Arizona [ http://science.opi.arizona.edu/ ]) noticed the moon when comparing a 1986 photo to a recent [ http://oposite.stsci.edu/pubinfo/pr/1998/35/index.html ] one taken by the Hubble Space Telescope [ http://www.stsci.edu/hst/ ]. The newly identified moon is hard to see but marked in the above photograph [ http://science.opi.arizona.edu/lasso.acgi?-database=science.fp3&-layout=Fields&-response=%2f%7escience%2fcurrentdetails.htm&-recid=34354&-search ]. Also visible are many other Uranian moons [ http://www.seds.org/nineplanets/nineplanets/uramoons.html ] and background stars. The moon is the 18th known around Uranus [ http://www.hawastsoc.org/solar/eng/uranus.htm ], tying it with Saturn [ http://www.seds.org/nineplanets/nineplanets/saturn.html ] for the most around any planet. |
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Two Hours Before Neptune
| Title |
Two Hours Before Neptune |
| Explanation |
Two hours before closest approach to Neptune [ http://www.seds.org/nineplanets/nineplanets/neptune.html ] in 1989, the Voyager 2 [ http://vraptor.jpl.nasa.gov/voyager/vgrfaqs.html ] robot spacecraft snapped this picture [ http://nssdc.gsfc.nasa.gov/photo_gallery/photogallery-neptune.html ]. Clearly visible for the first time were long light-colored cirrus [ http://earthsky.worldofscience.com/1998/es980706.html ]-type clouds floating high in Neptune's atmosphere [ http://nssdc.gsfc.nasa.gov/photo_gallery/caption/neptune_clouds.txt ]. Shadows of these clouds can even be seen on lower cloud decks. Most of Neptune's atmosphere [ http://antwrp.gsfc.nasa.gov/apod/ap960507.html ] is made of hydrogen [ http://chemlab.pc.maricopa.edu/periodic/h.html ] and helium [ http://chemlab.pc.maricopa.edu/periodic/He.html ], which is invisible. Neptune's blue color therefore comes from smaller amounts of atmospheric methane [ http://www.epa.gov/ghginfo/ ], which preferentially absorbs red light. Neptune [ http://pds.jpl.nasa.gov/planets/welcome/neptune.htm ] has the fastest winds in the Solar System [ http://www.seds.org/nineplanets/nineplanets/overview.html ], with gusts reaching 2000 kilometers per hour. Recent speculation [ http://www.urel.berkeley.edu/urel_1/CampusNews/PressReleases/releases/9-30-1999a.html ] holds that diamonds [ http://www.sdnhm.org/exhibits/diamonds/facts.html ] may be created in the dense hot conditions that exist under the clouds-tops of Uranus [ http://spacelink.msfc.nasa.gov/Instructional.Materials/Curriculum.Support/Space.Science/Our.Solar.System/Uranus/ ] and Neptune. |
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