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| | | title = Oort Cloud | | | title = Oort Cloud |
| | | image = oort_cloud.png | | | image = oort_cloud.png |
| − | | titletext = ...I wanna try. Hang on, be right back. | + | | titletext = ... I wanna try. Hang on, be right back. |
| | }} | | }} |
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| | ==Explanation== | | ==Explanation== |
| − | The {{w|Oort cloud}} is a hypothesized sphere containing many {{w|small Solar System bodies}}, reaching out to roughly 50,000 {{w|Astronomical unit|AU (astronomical units)}} or nearly one {{w|light-year}} from the sun. Gravitational forces from passing stars or collisions with other objects sometimes perturb one of these bodies enough to let it fall into the inner solar system. When it gets closer to the Sun, which is just a bright dot at that far distance, it warms up and some of its mass is lost as gas and dust, making it more visible as an object commonly referred to as a comet. This is what has happened to a comet called {{w|C/2013 UQ4}}, AKA Comet Catalina. And although this is not what will happen to Catalina, comets that get close enough to the sun may break up entirely. | + | {{incomplete|Not (yet) complete.}} |
| | + | The {{w|Oort cloud}} is a cloud mostly composed of comets that makes up the outer region of our solar system, reaching out to roughly 50,000 [http://en.wikipedia.org/wiki/Astronomical_unit AU] or nearly one light-year from the sun. Gravitational forces from passing stars and the Milky Way sometimes perturb a comet enough to send it into the inner solar system. When the comet gets closer to the Sun (which is the “bright dot in the distance” here) it warms up and some of its body is lost as gas and dust, sometimes visible as a coma and perhaps a tail. If it gets close to the sun it may break up entirely. |
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| − | There seems to be no definitive astronomical definition of the word "comet", and definitions can be challenging and problematic [http://suitti.livejournal.com/56460.html?nojs=1], but in general terms a comet is a celestial object consisting of a nucleus containing a huge amount of ices and dust which, when near the sun, has an atmosphere (called {{w|Comet#Coma and tail|coma}}) and perhaps a 'tail' of ionized gas and dust particles pointing away from the sun.
| + | The comet pictured here upon its return resembles the unusual asteroid/comet {{w|P/2013 P5}} which sported six comet-like tails. In that case they seem to have been generated partly by rapid spinning. |
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| − | The comet pictured here upon its return strangely resembles the unusual asteroid {{w|P/2013 P5}}. That object sported six comet-like tails, but it's not a comet. Rather, the six comet-like tails were suspected to be caused by rapid spinning of that object.
| + | {{w|Comet ISON}} came from the Oort cloud and reached its closest approach to the sun ({{w|perihelion}}) on the day before this comic was published. The comet passed very close to the sun, at a distance of 1,860,000 kilometers or 1,150,000 miles. It was thus within one sun-diameter of the surface of the sun itself (diameter of sun = 1,391,000 km). The tail has changed its shape because the comet was partly broken up around the sun. The closest approach to Earth will be on December 27, 2013 but it's not clear if the comet will be visible by the naked eye. |
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| − | Randall has drawn the hapless Oort Cloud object with its tails generally left of frame, i.e. away from the sun. Comet tails point away from the sun regardless of their direction of movement, as they are blown out by the solar wind which moves much faster than the comet. As neither of the other two objects have tails, this lends the picture a comical cartoon-like quality, as when Yosemite Sam is blasted by his own gun and it leaves his mustache tails statically pointing away from the direction of the blast.
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| − | {{w|C/2012 S1|Comet ISON}} presumably came from the Oort cloud and reached its closest approach to the sun ({{w|Apsis|perihelion}}) on the day before this comic was published. The comet passed very close to the sun, at a distance of 1,860,000 kilometers or 1,150,000 miles from the center of the sun. It was thus within one sun-diameter of the surface of the sun itself (diameter of sun = 1,391,000 km). At that distance the temperature, at approx. 2,700 degrees Celsius, vaporizes rock as well as ice and can break the comet apart entirely. | |
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| − | The broken-up object here is presumed to be ISON, and is labeled as such in the transcript, even though Randall hasn't unambiguously identified it. Note that it's not realistic that ISON still would have a tail so far away from the sun.
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| − | On December 2, 2013 NASA released a statement that ISON did not survive its close perihelion with the sun. The Comet ISON Observing Campaign posted a delightful biographical sketch (In Memoriam Comet C/2012 S1 (ISON) Born 4.5 Billion BC, Fragmented Nov 28, 2013, age 4.5-billion yrs old) which touches on its early years, retreat to the Oort Cloud, career as a Sungrazer, "dynamic and unpredictable life, alternating between periods of quiet reflection and violent outburst", delicate inner working, and its tragic demise.
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| − | The closest approach of ISON to the earth was predicted for December 27, 2013 at a distance at approx. 60 million kilometers or 37 million miles, 170 hundred times more than the moon. The {{w| Hubble Space Telescope}} [http://www.universetoday.com/107407/hubble-looks-but-finds-no-trace-of-comet-ison/ looked for it on December 18] but saw nothing. | |
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| | This video shows an animation of the encounter at the sun: [http://stereo-ssc.nascom.nasa.gov/browse/2013/11/28/ahead_20131128_cor2_rdiff_512.mpg ISON 28.11.2013]. | | This video shows an animation of the encounter at the sun: [http://stereo-ssc.nascom.nasa.gov/browse/2013/11/28/ahead_20131128_cor2_rdiff_512.mpg ISON 28.11.2013]. |
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| − | ===Perspective===
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| − | Some more information about comets will help put the comic in perspective:
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| − | *The surface of cometary nuclei reflects less sunlight than asphalt. Telescopes can't identify or find them until they have a coma.
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| − | *An object at a distance of one light-year would only have an orbital speed about 100 meters per second; the speed of the Earth is about 30 kilometers per second.
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| − | *One revolution at that distance would last approximately 20 million years.
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| | ==Transcript== | | ==Transcript== |
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| | :[Pause while ISON checks it out off screen.] | | :[Pause while ISON checks it out off screen.] |
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| − | :ISON (broken up, with multiple tails): Wow. Do '''''NOT''''' go over there. | + | :[Several million years later.] |
| − | | + | :ISON (appears burnt): Wow. Do NOT go over there. |
| | {{comic discussion}} | | {{comic discussion}} |
| | [[Category:Astronomy]] | | [[Category:Astronomy]] |
