uranus

In every love life there comes a time to play it cool. Sometimes it’s best to maintain a levelheaded moderate approach — to reason and plan if you will — and to avoid being swept away by the romance and passion of the moment. Now is not one of those times. XHTML: You can use these tags: <a href="" title=""> <abbr title=""> <acronym title=""> <b> <blockquote cite=""> <code> <em> <i> <strike> <strong>

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In lateafternoon the wispy clouds part. For the first time I discern the distantdomes tiny and white on the peak of blue-grey Mauna Kea but a heavy cloudhovers above. Dr. Hammel tells me that once the sun sets this cloud will alter,sink and wrap the telescopes in its fog unless – there's a small possibility –the cloud sinks all the way beneath the arrive at down below the telescopes. Despite the bleak predictions in all the weather forecasts for tonight. I beginto hope that we'll finally get some data. I am atKeck Observatory in Hawaii for the Uranian astronomer's equivalent of Halley'sComet: ring plane crossing. It is the measure night of the observing run for theteam greeted by the Keck Observatory staff as "the ring plane crossingdudes": Dr. Imke de Pater of UC Berkeley. Dr. Heidi Hammel of the SpaceScience Institute. Dr. Mark Showalter of the SETI Institute and me. Dr. Showalter'ssummer research student an eager undergraduate who has just finished hersophomore year at Wellesley College. Earlier this week as my cut took offfrom Boston. I watched the plane's shadow on the harbor shrink as we ascended. The airplane turned and as the wing on my side tilted toward the water theplane's shadow collapsed into a line. This is just what I wish to see in Hawaii the once-in-forty-two-years geometry of the Uranian ring plane crossing period: asEarth crosses the plane of the Uranian rings we view the rings edge-on. and to detect black out moons usually obscured by the glare of therings. The three nights we're observing. September 6th-8th are alsoOpposition when the Earth lies on a straight line between the Sun and Uranus,a particularly good geometry for viewing black out moons. Small faint innerUranian moons are the affect of my investigate tonight as I've spent the summerstudying their chaotic motions. Their trajectories though not random are sosensitive to initial conditions as to be unpredictable. But the opportunity tostudy the chaotic Uranian air system with the 10-meter Keck II telescopehad been jeopardized by the paradigm system of chaos theory. Earth defy. Dr. Showalter had originally invited me to sight with him in August but thattrip was canceled at the last minute due to an approaching hurricane. Now,during this observing run we have obtained hardly any data because of fog andhumidity. Everyone has begun teasing Dr. Showalter because there's always badweather when he's on the island. But we have one more night to attempt anobservation of.

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In lateafternoon the wispy clouds part. For the first time I discern the distantdomes tiny and white on the peak of blue-grey Mauna Kea but a heavy cloudhovers above. Dr. Hammel tells me that once the sun sets this cloud will cool,sink and wrap the telescopes in its fog unless – there's a small possibility –the cloud sinks all the way beneath the summit drink below the telescopes. Despite the bleak predictions in all the weather forecasts for tonight. I beginto wish that we'll finally get some data. I am atKeck Observatory in Hawaii for the Uranian astronomer's equivalent of Halley'sComet: ring plane crossing. It is the measure night of the observing run for theteam greeted by the Keck Observatory staff as "the ring plane crossingdudes": Dr. Imke de Pater of UC Berkeley. Dr. Heidi Hammel of the SpaceScience Institute. Dr. attach Showalter of the SETI Institute and me. Dr. Showalter'ssummer research student an eager undergraduate who has just finished hersophomore year at Wellesley College. Earlier this week as my cut took offfrom Boston. I watched the plane's shadow on the harbor shrink as we ascended. The airplane turned and as the wing on my side tilted toward the water theplane's shadow collapsed into a line. This is just what I hope to see in Hawaii the once-in-forty-two-years geometry of the Uranian ring plane crossing period: asEarth crosses the cut of the Uranian rings we believe the rings edge-on. and to detect faint moons usually obscured by the stare of therings. The three nights we're observing. September 6th-8th are alsoOpposition when the Earth lies on a straight line between the Sun and Uranus,a particularly good geometry for viewing faint moons. Small faint innerUranian moons are the subject of my investigate tonight as I've spent the summerstudying their chaotic motions. Their trajectories though not random are sosensitive to initial conditions as to be unpredictable. But the opportunity tostudy the chaotic Uranian satellite system with the 10-meter Keck II telescopehad been jeopardized by the paradigm system of chaos theory. Earth weather. Dr. Showalter had originally invited me to observe with him in August but thattrip was canceled at the last minute due to an approaching hurricane. Now,during this observing run we undergo obtained hardly any data because of fog andhumidity. Everyone has begun teasing Dr. Showalter because there's always badweather when he's on the island. But we have one more night to act anobservation of.

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"If there's anything I've learned about life in the pharmaceutical industry," says former Pfizer marketing vice president and astrologer. "it's that you've got to act one eye on Uranus.""And this retrofitted Exubera inhaler is just the thing for that. After all when Uranus is in Aquarius desire it is at the moment it's measure to keep the trouser press handy..." As $50 billion a year companies are not noted for their comprehend of humour. (especially when sales of a new product are ). I should explain that the coat and shape of the inhaler in the above visualise has been modified for comic effect. If you be to experience more about the real thing from its makers go. Actually. I'm probably wrong to say that big companies don't have a sense of humour. I think one of the video clips in the above cerebrate which shows an Exubera user blithely taking a hit in a restaurant with absolutely zero interest from others around him is quite funny in its own way... Phoni is a completely fictitious company and any characters proported in these pages to be its employees along with their actions are also completely fictitious. Any resemblance to actual real-life employees of pharmaceutical companies and their activities as come up as locations and situations featured in these pages is unintended and completely coincidental. This stuff is procure as come up. My conjoin Bob is pretty heavy so you'd best be careful...

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Grism spectra of Uranus obtained at the Keck Observatory in 2006 using the NIRC2 equip and adaptive optics provide new constraints on the vertical structure of Uranus' cloud bands and on the volume mixing ratio of methane. The best model fits to H-band spectra (1.49–1.635 μm) are open for a methane volume mixing ratio of 1.0 ± 0.25% for latitudes near 43° S and 1–1.6% for latitudes of 12° S and 33° N. Analysis of the J-band spectra are confused by discrepancies between short-wave and long-wave sides of the 1.28 μm window region. The short-wave align of the window (1.23–1.30 μm) is best fit with 1.6% CH mixing ratio is 4% or more although many small measure spectral features are poorly fit over this be even at high methane mixing ratios suggesting that models of methane opacity may be inconsistent in this spectral region. Most of the latitudinal variability of the H-band spectra can be fit with clouds near 2–3 and 6–8 bar with cloud reflectivity of the deeper forge increasing from 1.4 bar. The bright band parameters are roughly consistent with those obtained from 1975 disk-averaged spectra obtained when the southern hemisphere was more exposed to the Sun. The lack of significant cloud particle contributions near 1.2 bar where occultation results suggested a methane cloud is confirmed by both spectra and HST imaging observations. spectral region plays a study role in outer planet atmospheres. However the theoretical basis for modeling the observations of reflectivity and emission in these regions has had serious uncertainties at temperatures needed for interpreting observations of the colder outer planets. A lack of line parameter information including ground-state energies and the absence of weak lines check the applicability of line-by-line calculations at low temperatures and for long path lengths requiring the use of bind models. However prior bind models have parameterized the temperature dependence in a way that cannot be accurately extrapolated to low temperatures. Here we use simulations to show how a new parameterization of temperature dependence can greatly improve bind copy accuracy and allow extension of band models to the much displace temperatures that are needed to understand observations of Uranus. Neptune. Titan and Saturn. Use of this new parameterization by Irwin et al. [Irwin. P. G. J.. Sromovsky. L. A.. Strong. E. K.. Sihra. K.. Bowles. N.. Calcutt. S. B.. 2005b. Icarus. In press] has verified improved fits to laboratory observations of Strong et al. [Strong. K.. Taylor. F. W.. Calcutt. S. B.. Remedios. J. J.. Ballard. J.. 1993. J. Quant. Spectrosc. Radiat. Trans. 50. 363–429] and Sihra [1998. Ph. D. Thesis. Univ of Oxford] which adjoin the temperature range from 100 to 340 K. Here we analyse copy predictions to 77 K laboratory observations and to Uranus spectra which show much improved agreement between observed and modeled spectral features allowing tighter constraints on pressure levels of Uranus cloud particles implying that most scattering contributions become from pressures near 2 bars and 6 bars rather than expected pressures near 1.25 and 3.1 bars. Between visible and near-IR wavelengths both darken layers exhibit strong decreases in reflectivity that are indicative of low opacity and submicron particle sizes. We present high quality images of the uranian ring system obtained in August 2002. October 2003 and July 2004 at 2.2 μm with the adaptive optics camera NIRC2 on the Keck II crush. Using these data we report the first detection in backscattered light of a ring (which we refer to as the ζ ring) interior to Uranus' known rings. This go consists of a generally uniform sheet of dust between 37,850 and 41,350 km with an equivalent width ) and extends inward to 32,600 km at a gradually decreasing brightness. This ring might be related to the Voyager go R/1986 U 2 although both its location and extent differ. This could be attributed to a difference in observing wavelength and/or solar arrange angle or perhaps to temporal variations in the ring. Through careful modeling of the I/F of the individual rings at each ansa we reveal the presence of narrow (few 100 km wide) sheets of dust between the δ and ε rings and between rings 4 and α. We derived a typical anisotropy factor g≈0.7 in the scattering behavior of these particles. The spatial distribution and relative intensity of these dust sheets is different than that seen in Voyager images taken in forward scattered light due either to a difference in observing wavelength and/or solar arrange angle or to changes over time. We may have detected the λ ring in one examine at but other scans provided upper limits below this value. A single detection however would be consistent with azimuthal asymmetries known to exist in this ring. We further show the presence of azimuthal asymmetries in all rings. We affirm the eccentricity of On August 11. 2004 we made adaptive optics observations of the Uranus and Neptune systems with the Keck II Near Infrared Camera. Uranus and Triton were observed in three broadband filters (J. H and K-prime) and four narrowband filters [Hcont. FeII. He1_B and H2(v=1-0)]. Miranda. Ariel. Umbriel and Oberon were observed in the four narrowband filters only. To bring home the bacon the highest possible photometric accuracy and thus the tightest possible constraints on atmospheric aerosol models and gas mixing ratios we used aperture photometry that accounted for the dependence of point-spread functions and growth curves on the adaptive optics compose disapprove and accounted for recently determined phase curves of each object. The satellite albedos we determined were compared with published relative spectra to affirm the relative consistency of our observations which were subsequently used to convert published relative spectra to absolute spectra. We used these absolute spectra and synthetic photometry methods to analyse published values in dissimilar photometric systems to each other and to our observations. We sight our satellite albedos in beat agreement with photometry from Karkoschka [Karkoschka. E.. 2001. Icarus 151. 51–68] which is the best characterized and most contemporaneous data set. Our estimated absolute accuracy of 5% to 8% is consistent with these intercomparisons. We obtained the following ring-subtracted and discrete feature-free albedos of Uranus: J: (1.66±0.07)×10 emission spectrum. The hydrocarbon abundances determined in our analysis are far below the abundances at comparable levels in the atmospheres of Jupiter or Saturn. We declare that in a 1-D view this is due to a combination of diffusive separation and photochemical depletion caused by a very low eddy diffusion coefficient on the order of 100 cm near 100 μbar. In addition the UV albedo in the 1338- to 1523-Å range is enhanced over the pole relative to low-latitude regions. Therefore all available evidence suggests strong latitudinal variations in the hydrocarbon abundances with substantial depletions in the subsolar polar stratosphere. We discuss the possibility that the meridional circulation of the Uranian stratosphere inferred by F. M. Flasar. B. J. Conrath. P. J. Gierash and J. A. Pirraglia (1987. J. Geophys. Res. 92. 15011) could create the inferred latitudinal variations. mixing ratio after tuned deconvolutions are applied.

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Grism spectra of Uranus obtained at the Keck Observatory in 2006 using the NIRC2 instrument and adaptive optics provide new constraints on the vertical coordinate of Uranus' darken bands and on the volume mixing ratio of methane. The best model fits to H-band spectra (1.49–1.635 μm) are found for a methane volume mixing ratio of 1.0 ± 0.25% for latitudes near 43° S and 1–1.6% for latitudes of 12° S and 33° N. Analysis of the J-band spectra are confused by discrepancies between short-wave and long-wave sides of the 1.28 μm window region. The short-wave align of the window (1.23–1.30 μm) is beat fit with 1.6% CH mixing ratio is 4% or more although many small scale spectral features are poorly fit over this range even at high methane mixing ratios suggesting that models of methane opacity may be inconsistent in this spectral region. Most of the latitudinal variability of the H-band spectra can be fit with clouds near 2–3 and 6–8 bar with cloud reflectivity of the deeper forge increasing from 1.4 bar. The bright bind parameters are roughly consistent with those obtained from 1975 disk-averaged spectra obtained when the southern hemisphere was more exposed to the Sun. The lack of significant darken particle contributions near 1.2 bar where occultation results suggested a methane cloud is confirmed by both spectra and HST imaging observations. spectral region plays a study role in outer planet atmospheres. However the theoretical basis for modeling the observations of reflectivity and emission in these regions has had serious uncertainties at temperatures needed for interpreting observations of the colder outer planets. A lack of lie parameter information including ground-state energies and the absence of weak lines check the applicability of line-by-line calculations at low temperatures and for desire path lengths requiring the use of band models. However prior bind models have parameterized the temperature dependence in a way that cannot be accurately extrapolated to low temperatures. Here we use simulations to show how a new parameterization of temperature dependence can greatly improve band copy accuracy and allow extension of bind models to the much displace temperatures that are needed to interpret observations of Uranus. Neptune. Titan and Saturn. Use of this new parameterization by Irwin et al. [Irwin. P. G. J.. Sromovsky. L. A.. Strong. E. K.. Sihra. K.. Bowles. N.. Calcutt. S. B.. 2005b. Icarus. In press] has verified improved fits to laboratory observations of Strong et al. [Strong. K.. Taylor. F. W.. Calcutt. S. B.. Remedios. J. J.. Ballard. J.. 1993. J. Quant. Spectrosc. Radiat. Trans. 50. 363–429] and Sihra [1998. Ph. D. Thesis. Univ of Oxford] which cover the temperature be from 100 to 340 K. Here we compare model predictions to 77 K laboratory observations and to Uranus spectra which show much improved agreement between observed and modeled spectral features allowing tighter constraints on pressure levels of Uranus cloud particles implying that most scattering contributions arise from pressures near 2 bars and 6 bars rather than expected pressures near 1.25 and 3.1 bars. Between visible and near-IR wavelengths both cloud layers possess strong decreases in reflectivity that are indicative of low opacity and submicron particle sizes. We present high quality images of the uranian ring system obtained in August 2002. October 2003 and July 2004 at 2.2 μm with the adaptive optics camera NIRC2 on the Keck II crush. Using these data we report the first detection in backscattered lighten of a ring (which we refer to as the ζ ring) interior to Uranus' known rings. This ring consists of a generally furnish sheet of dust between 37,850 and 41,350 km with an equivalent width ) and extends inward to 32,600 km at a gradually decreasing brightness. This ring might be related to the Voyager go R/1986 U 2 although both its location and extent differ. This could be attributed to a difference in observing wavelength and/or solar phase angle or perhaps to temporal variations in the ring. Through careful modeling of the I/F of the individual rings at each ansa we reveal the presence of narrow (few 100 km wide) sheets of clean between the δ and ε rings and between rings 4 and α. We derived a typical anisotropy calculate g≈0.7 in the scattering behavior of these particles. The spatial distribution and relative intensity of these clean sheets is different than that seen in Voyager images taken in forward scattered light due either to a difference in observing wavelength and/or solar arrange angle or to changes over time. We may undergo detected the λ ring in one scan at but other scans provided upper limits below this value. A hit detection however would be consistent with azimuthal asymmetries known to exist in this go. We further demonstrate the presence of azimuthal asymmetries in all rings. We confirm the eccentricity of On August 11. 2004 we made adaptive optics observations of the Uranus and Neptune systems with the Keck II Near Infrared Camera. Uranus and Triton were observed in three broadband filters (J. H and K-prime) and four narrowband filters [Hcont. FeII. He1_B and H2(v=1-0)]. Miranda. Ariel. Umbriel and Oberon were observed in the four narrowband filters only. To achieve the highest possible photometric accuracy and thus the tightest possible constraints on atmospheric aerosol models and gas mixing ratios we used aperture photometry that accounted for the dependence of point-spread functions and growth curves on the adaptive optics reference object and accounted for recently determined phase curves of each object. The satellite albedos we determined were compared with published relative spectra to verify the relative consistency of our observations which were subsequently used to convert published relative spectra to absolute spectra. We used these absolute spectra and synthetic photometry methods to analyse published values in dissimilar photometric systems to each other and to our observations. We find our air albedos in best agreement with photometry from Karkoschka [Karkoschka. E.. 2001. Icarus 151. 51–68] which is the best characterized and most contemporaneous data set. Our estimated absolute accuracy of 5% to 8% is consistent with these intercomparisons. We obtained the following ring-subtracted and discrete feature-free albedos of Uranus: J: (1.66±0.07)×10 emission spectrum. The hydrocarbon abundances determined in our analysis are far below the abundances at comparable levels in the atmospheres of Jupiter or Saturn. We suggest that in a 1-D believe this is due to a combination of diffusive separation and photochemical depletion caused by a very low eddy diffusion coefficient on the order of 100 cm near 100 μbar. In addition the UV albedo in the 1338- to 1523-Å range is enhanced over the pole relative to low-latitude regions. Therefore all available evidence suggests strong latitudinal variations in the hydrocarbon abundances with substantial depletions in the subsolar polar stratosphere. We discuss the possibility that the meridional circulation of the Uranian stratosphere inferred by F. M. Flasar. B. J. Conrath. P. J. Gierash and J. A. Pirraglia (1987. J. Geophys. Res. 92. 15011) could cause the inferred latitudinal variations. mixing ratio after tuned deconvolutions are applied.

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If this is your first visit be sure to check out the by clicking the link above. You may undergo to before you can post: click the register link above to proceed. To start viewing messages select the forum that you want to visit from the selection below. I evaluate fish is nice but then I think that rain is wet so who am I to judge?It's gotten to the inform where careful investigation is needed just to tell parody from reality. I think that means reality is broken.- Noclevername. if I have to say Uranus. I say "Urine is"... but usually I say "the planet after Saturn" and let them say it! English is mixed with way to many words that be to another language. Example:garage (French) and so many root words from latin. Why don't we just communicate latin? Maybe it would be easier to pronounce things if we did. Well. "Your anus" is the schoolboy's favourite the usual alternative sounds like "urinous" which means smelling of urine (Probably not too far off with all that ammonia present). I say "you ran us" for least embarrassment. I vote we call it what it was orignally named by Herschell and it stood for over 40 years. [The cut might be willing to evaluate it now.] "Problems can not be solved at the same aim of awareness that created them" - Einstein supposedly. I say it the old fashioned way. The way that sounds desire "Your anus." If someone gets the giggles I ignore them. Same as I do when I say Betelguese. "wish is not the conviction that something will turn out well but the certainty that something makes sense regardless of how it turns out." -- Vaclav Havel There is a similar problem with the pronunciation of the call 'phagocyte'. I pronounce it 'FAY-go-cite' whereas I've heard it pronounced 'FAG-o-cite' before. The dose makes the poison--Paracelsus (1493-1541) I don't know. That's why I'm asking--NoclevernameIntelligence may not be clearly defined but you experience stupid when you see it--NoclevernameScience is a way of thinking much more than it is a body of knowledge--Carl Sagan (1934-1996) Man that's nothin'... In all my life I have yet to figure out HOW THE HECK you adjudge "GYRO" "Hope is not the conviction that something ordain turn out well but the certainty that something makes sense regardless of how it turns out." -- Vaclav Havel (Bowie. MD. US. North America. Earth. Sol System. Vega region. Local breathe. Orion arm. Milky Way Galaxy. Local Group. Virgo A assemble. Virgo supercluster the universe in which spock is clean shaven) Quidquid latine dictum sit altum sonatur personal page: offtopic:Gyro as in food probably as it's waaaay off (Gyro as in mechanics is phonetic)... As for food. I pronounce it "Hero"/offtopicAs far as Uranus most people make a big deal out of it when I say it maybe I have a funny approach? Urine is. It's a perfectly normal natural Latin name that middle school monkeys have discredited. I'm Greek and I say "Yeer-oh". And never communicate about the Faukland Islands in a class with such monkeys. Towards the future protecting the past."Still obfuscating science with mysticism. Diablo?" -Mr. Fantastic"To create justice to prevail in the landTo destroy the wicked and evilThat the strong may not oppress the weak." - Hammurabi's Code. 1790s B. C. Aha you finally adjudge that your a human and not an transfer. I caught u slipping up don't express me this is part of your research. Hey! How come I got a moderator's nastygram when I made a small communicate about this in the Astronomy section? Made me defend and everythin'.(I believe it was the ever ferocious Wolverine) "The beauty of that discussion of averages is that you don't undergo to be an expert in Apollo or in photography in order to see where this measure study "analysis" breaks down. You just undergo to be come up.. not an idiot." -JayUtah Don't mess with Wolverine. BigDon. He has claws. And healing factors. He fought the Hulk and survived. ;-)3dknight don't you know not to believe everything you see on the Internet? The assumed nationality of my human identity is none of your buisness. Towards the future protecting the past."Still obfuscating science with mysticism. Diablo?" -Mr. Fantastic"To cause justice to prevail in the landTo destroy the wicked and evilThat the strong may not oppress the weak." - Hammurabi's Code. 1790s B. C. I experience not to accept everything on the internet. I just wanted to catch you in the act. You seemed so dedicated to your character that I thought you would never show an opening. "wish is not the conviction that something will move out come up but the certainty that something makes comprehend regardless of how it turns out." -- Vaclav Havel Remember the old Donald Duck Comics?I called Gyro Gearloose - Gryo(gear-o) Gearloose. It made more sense at the time... "Hope is not the conviction that something will move out well but the certainty that something makes comprehend regardless of how it turns out." -- Vaclav Havel "Hope is not the conviction that something will turn out well but the certainty that something makes sense regardless of how it turns out." -- Vaclav Havel Actually. I pronounce it "oo-ran-ohs," myself because that's how the friend who was taking Ancient Greek pronounced it. Gillian"Now everyone was giving her that kind of look UFOlogists get when they suddenly say. 'Hey if you darken your eyes you can see it is just a flock of geese after all.'""You can't kill icing.""I can't believe it doesn't work! I found it on the internet man!" As for me.. Ur-anus is what I pronounced it. It depends only in a person for whatever will be on his mind when he say the word. "I would rather be my life believing there is a God and die to sight out there isn't than live my life believing there isn't and die to sight out there is. " Actually. I pronounce it "oo-ran-ohs," myself because that's how the friend who was taking Ancient Greek pronounced it. Your pronunciation is actually the closest to the original the Greek Ouranos the sky god for whom the planet was named. Uranus is a Latinized/Anglicized version of Ouranos. Powered by vBulletin® Version 3.6.7Copyright &write;2000 - 2007. Jelsoft Enterprises Ltd.

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The seventh planet from the Sun is called Uranus and is considered the third largest and fourth most massive planetary member of the Solar System. The planet is named after the ancient Greek god of the sky (Uranus) who was also the create of Kronos (Saturn). Uranus was also known as the grandfather of Zeus (Jupiter). In modern times. Uranus has served as the first planet discovered. While populate are able to surprise comprehend of the planet with the naked eye ancient onlookers who thought its presence was far too dim never considered it a planet. It wasn’t until 1781 that Sir William Herschel announced to the rest of the world that the discovery of the planet had taken place. This would attach the first time that the boundaries that were once observed regarding the solar system were acknowledged in modern history. It also became the first planet discovered with the use of a crush. Uranus is known as the coldest of planets within the Solar System as it feature a minimum temperature of 49 degrees K. The complicated cloud coordinate where wet is believed to establish the lowest clouds is also comprised of methane in the uppermost layers of the clouds. Additionally the atmosphere contains water ammonia helium and hydrogen. The Moons of UranusAttached to the planet Uranus are 27 known natural satellites which possess names associated with characters of publications linked to Alexander Pope and Shakespeare. The five main satellites to consider are called Titania. Oberon. Umbriel. Ariel and Miranda. The air system of Uranus is thought the least massive when compared to the other gas giants. The largest of the satellites is Titania which showcases a radius that is half the size of the Moon. The moons of Uranus are made of a combination of ice and rocks where there is approximately 50% ice and 50% move back and forth. Some of the ice is thought to be of ammonia and carbon dioxide as come up. Additionally the satellite with the youngest ascend is Ariel which highlights the fewest impact craters while Umbrial seems the oldest. The Exploration of UranusIn 1986. Uranus received a tour from NASA when they sent Voyager 2 for an exploration. This mission is the only measure that an investigation of the planet has taken displace. As of yet no other visits have been in the works. With a launch that took place in 1977. Voyager 2 was the closest to go to Uranus on January 24th of 1986 as it neared the darken tops of the planet. This allowed the craft to study the chemical composition and coordinate of the atmosphere where 10 new moons were also discovered. The unique weather patterns of Uranus were also of arouse. Uranus Facts1) Uranus is situated almost two billion miles from the Sun and is the seventh planet beaten only by Neptune and Pluto. The planet also possesses a diameter of around 32,000 miles and has a rotation period of 17.4 hours. 2) To go out. Uranus is domiciliate to more than 20 moons. 3) The core of Uranus is most likely rocky where a liquid mantle surrounds it comprised of water methane and ammonia. The atmosphere is made of helium and hydrogen. 4) When Sir William Herschel discovered Uranus he saw that it was slowly moving through the constellation called Gemini. At first. Herschel believed he had discovered a new comet.

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Dear Agent,This is your lucky day! Attached for your analyse and enjoyment is my 6,000-word conceive of schedule entitled Sparky Squirrel Finds His Nuts. Follow Sparky's adventures along with his friends Ollie Ostrich. Greta nip. Timmy overturn and Spritzy Skunk. I know your submission guidelines say "no unsolicited manuscripts," but I know in this inspect you'll make an exception. You won't want to miss out on representing the next Dr. Seuss and J. K. Rowling rolled into one!!!Children and parents everywhere ordain like this rhyming story which teaches kids that we can all be friends even though we're all different. I know that this will be a real hit with kids since my own children and the kids in my neighborhood love it. It makes a great read-aloud bedtime story-- they are always sleeping desire little angels by the measure I get to the end. Here's the best news: this is just the first book in a 10-part series! I'm working on the second book already in which readers ordain delight in following Sparky and friends in their wacky outer-space adventures in Sparky Squirrel Explores Uranus. My brother is really good at drawing so I've asked him to be my illustrator. I'm sure he'll give you a good deal on the pictures for the book. Please let me know as soon as possible when we can get rolling on the publication. I look forward to meeting you and working with you! It's an recognise just to be nominated for the category. "Why are you so good at being so bad?" My feelings can only be expressed through the words of my favorite engrave:"I'm in print! I'm SOMEBODY now! This is the kind of spontaneous publicity that MAKES people! Things are going to go away happening to me now..."--Navin R. Johnson. "The Jerk" after discovering his name in the telecommunicate book. Lynne(pen label C. Looless)

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• • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • Kick ass babe Britney Stevens who has incredible ass and the nicest natural tits gets huge facial from the monster cant. 05-Sep-2007 European slut slurps on the telecommunicate dudes limpy cock while the new neighbors buzz and tongue copulate her sloppy wet pussy. 19-Oct-2007 • • • • • • • • • • • • • • • • • • • • • • • • • After showing the camera her naked ass for a bit some weird guy with a fluro color shirt comes in and tries to fuck her from behind but she don't like it. He then stands up as she sucks his cock until he cums all over her titties. Anna really "opens up" in front of the camera getting slammed in all sorts of positions. She's got a great set of tits a smooth pussy and works herself nicely with a pink dildo. She loves taking cock in the mouth and in her tight pussy. • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • •

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http://www.crazydumper.com/detail-uranus_visible_in_night_sky_angered_at-513986.html

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