{
  "submission_id": "1888000",
  "keywords": [
    {
      "keyword_id": "475009",
      "keyword_name": "astrophysics",
      "contributed": "f",
      "submissions_count": "1"
    },
    {
      "keyword_id": "2591",
      "keyword_name": "science",
      "contributed": "f",
      "submissions_count": "2300"
    },
    {
      "keyword_id": "50041",
      "keyword_name": "wolfpup",
      "contributed": "f",
      "submissions_count": "12"
    }
  ],
  "hidden": "f",
  "scraps": "f",
  "favorite": "f",
  "favorites_count": "0",
  "create_datetime": "2019-05-19 21:52:41.468882+00",
  "create_datetime_usertime": "19 May 2019 23:52 CEST",
  "last_file_update_datetime": "2019-05-19 21:51:45.785548+00",
  "last_file_update_datetime_usertime": "19 May 2019 23:51 CEST",
  "username": "Yiffox",
  "user_id": "11477",
  "user_icon_file_name": "138471_Yiffox_yiffox_icons_6.jpg",
  "user_icon_url_large": "https://nl1.ib.metapix.net/usericons/large/138/138471_Yiffox_yiffox_icons_6.jpg",
  "user_icon_url_medium": "https://nl1.ib.metapix.net/usericons/medium/138/138471_Yiffox_yiffox_icons_6.jpg",
  "user_icon_url_small": "https://nl1.ib.metapix.net/usericons/small/138/138471_Yiffox_yiffox_icons_6.jpg",
  "file_name": "2715033_Yiffox_evolution_4.5.doc",
  "file_url_full": "https://nl1.ib.metapix.net/files/full/2715/2715033_Yiffox_evolution_4.5.doc",
  "file_url_screen": "https://nl1.ib.metapix.net/files/screen/2715/2715033_Yiffox_evolution_4.5.doc",
  "file_url_preview": "https://nl1.ib.metapix.net/files/preview/2715/2715033_Yiffox_evolution_4.5.doc",
  "files": [
    {
      "file_id": "2715033",
      "file_name": "2715033_Yiffox_evolution_4.5.doc",
      "file_url_full": "https://nl1.ib.metapix.net/files/full/2715/2715033_Yiffox_evolution_4.5.doc",
      "file_url_screen": "https://nl1.ib.metapix.net/files/screen/2715/2715033_Yiffox_evolution_4.5.doc",
      "file_url_preview": "https://nl1.ib.metapix.net/files/preview/2715/2715033_Yiffox_evolution_4.5.doc",
      "mimetype": "application/msword",
      "submission_id": "1888000",
      "user_id": "11477",
      "submission_file_order": "0",
      "full_size_x": null,
      "full_size_y": null,
      "screen_size_x": null,
      "screen_size_y": null,
      "preview_size_x": null,
      "preview_size_y": null,
      "initial_file_md5": "85ea20e92090e94cb2c2eac178c48203",
      "full_file_md5": "85ea20e92090e94cb2c2eac178c48203",
      "large_file_md5": "",
      "small_file_md5": "",
      "thumbnail_md5": "",
      "deleted": "f",
      "create_datetime": "2019-05-19 21:51:45.785548+00",
      "create_datetime_usertime": "19 May 2019 23:51 CEST"
    }
  ],
  "pools": [],
  "description": "this is just my own thoughts on matter and apparently I recorded them yay...I wanted to be astrophysicist when I grew up, screw u firemen...LITERALLY",
  "description_bbcode_parsed": "<span style='word-wrap: break-word;'>this is just my own thoughts on matter and apparently I recorded them yay...I wanted to be astrophysicist when I grew up, screw u firemen...LITERALLY</span>",
  "writing": "Even then, there is no process to distribute these heavier metals other than expansion of gas at sub-light speeds.  There is no known process to transfer these elements from the galactic bulge where the first supernovae are thought to occur.  Stars are incredibly far apart from each other, and yet science would have us believe that supernovae occurred relatively near every metal-rich star.  Furthermore, this would have to collide with gas that somehow is not accelerated away by the massive waves of gamma radiation that precede it.  This seems unlikely.\n\nThe quantity of added material may also be problematic.  Given that an expanding supernova most simply is a sphere of expanding matter, then:\n\nThe surface area of this sphere = 4?r2\n\nwhere r = the distance between the supernova core and the expanding sphere \n\nmeasured in light years.\n\nGiven that the general area of star formation tends to be around 2 light years, an effected area must penetrate a square of two light years by two light years or 4 square light years.\n\nSo the effective penetration of a supernova (p) =               = \n\nThus, a supernova four light years away would produce a penetration 1.99% of its expelled mass, which is around the distance of the closest star to the Sun.  One twenty five light years away would penetrate .159% of its expelled matter, while one a hundred light years away would only penetrate .0032%.  As the table below shows stars must be relatively near and massive to have a significant impact on spreading mass to nearby systems.  The average stellar mass is only .5 a solar mass so \n\n\t4ly - 1.99%\t25ly - .159%\t100ly - .0032%\n\n10SM\t.199 SM\t208.4 JpM\t.0159 SM\t16.7 JpM\t.00032 SM\t.335 JpM\n\n20SM\t.398 SM\t416.9 JpM\t.0318 SM\t33.3 JpM\t.00064 SM\t.67 JpM\n\n30SM\t.597 SM\t625.3 JpM\t.0477 SM\t50.1 JpM\t.00096 SM\t1.005 JpM\n\n40SM\t.796 SM\t833.7 JpM\t.0636 SM\t66.6 JpM\t.00128 SM\t1.34 JpM\n\n1 Jupiter mass (JpM) = @ .1% of our solar system\n\n  \n\n Mass of Jupiter [WWW]   HYPERLINK \"http://hypertextbook.com/facts/2002/DavidEngel.shtml\"  http://hypertextbook.com/facts/2002/DavidEngel.shtml  (April 23, 2008)\n\n Solar System [WWW]   HYPERLINK \"http://en.wikipedia.org/wiki/Solar_System\"  http://en.wikipedia.org/wiki/Solar_System  (April 23, 2008)\n\nAE\n\nE\n\nE\n\n\t\n\nz\n\n|\n\nE\n\nI\n\n\t\n\nN\n\nO\n\n http://www.astronomynotes.com/starprop/s2.htm  (April 23, 2008)\n\n1\n\n4\n\n?r2    \n\n4?r2\n\n",
  "writing_bbcode_parsed": "<span style='word-wrap: break-word;'>Even then, there is no process to distribute these heavier metals other than expansion of gas at sub-light speeds.&nbsp;&nbsp;There is no known process to transfer these elements from the galactic bulge where the first supernovae are thought to occur.&nbsp;&nbsp;Stars are incredibly far apart from each other, and yet science would have us believe that supernovae occurred relatively near every metal-rich star.&nbsp;&nbsp;Furthermore, this would have to collide with gas that somehow is not accelerated away by the massive waves of gamma radiation that precede it.&nbsp;&nbsp;This seems unlikely.<br /><br />The quantity of added material may also be problematic.&nbsp;&nbsp;Given that an expanding supernova most simply is a sphere of expanding matter, then:<br /><br />The surface area of this sphere = 4?r2<br /><br />where r = the distance between the supernova core and the expanding sphere <br /><br />measured in light years.<br /><br />Given that the general area of star formation tends to be around 2 light years, an effected area must penetrate a square of two light years by two light years or 4 square light years.<br /><br />So the effective penetration of a supernova (p) =&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; = <br /><br />Thus, a supernova four light years away would produce a penetration 1.99% of its expelled mass, which is around the distance of the closest star to the Sun.&nbsp;&nbsp;One twenty five light years away would penetrate .159% of its expelled matter, while one a hundred light years away would only penetrate .0032%.&nbsp;&nbsp;As the table below shows stars must be relatively near and massive to have a significant impact on spreading mass to nearby systems.&nbsp;&nbsp;The average stellar mass is only .5 a solar mass so <br /><br />\t4ly - 1.99%\t25ly - .159%\t100ly - .0032%<br /><br />10SM\t.199 SM\t208.4 JpM\t.0159 SM\t16.7 JpM\t.00032 SM\t.335 JpM<br /><br />20SM\t.398 SM\t416.9 JpM\t.0318 SM\t33.3 JpM\t.00064 SM\t.67 JpM<br /><br />30SM\t.597 SM\t625.3 JpM\t.0477 SM\t50.1 JpM\t.00096 SM\t1.005 JpM<br /><br />40SM\t.796 SM\t833.7 JpM\t.0636 SM\t66.6 JpM\t.00128 SM\t1.34 JpM<br /><br />1 Jupiter mass (JpM) = @ .1% of our solar system<br /><br />&nbsp;&nbsp;<br /><br />&nbsp;Mass of Jupiter [WWW]&nbsp;&nbsp; HYPERLINK &quot;<a href=\"http://hypertextbook.com/facts/2002/DavidEngel.shtml&quot;\" rel=\"nofollow\">http://hypertextbook.com/facts/2002/DavidEngel.shtml&q...</a>&nbsp;&nbsp;<a href=\"http://hypertextbook.com/facts/2002/DavidEngel.shtml\" rel=\"nofollow\">http://hypertextbook.com/facts/2002/DavidEngel.shtml</a>&nbsp;&nbsp;(April 23, 2008)<br /><br />&nbsp;Solar System [WWW]&nbsp;&nbsp; HYPERLINK &quot;<a href=\"http://en.wikipedia.org/wiki/Solar_System&quot;\" rel=\"nofollow\">http://en.wikipedia.org/wiki/Solar_System&quot;</a>&nbsp;&nbsp;<a href=\"http://en.wikipedia.org/wiki/Solar_System\" rel=\"nofollow\">http://en.wikipedia.org/wiki/Solar_System</a>&nbsp;&nbsp;(April 23, 2008)<br /><br />AE<br /><br />E<br /><br />E<br /><br />\t<br /><br />z<br /><br />|<br /><br />E<br /><br />I<br /><br />\t<br /><br />N<br /><br />O<br /><br />&nbsp;<a href=\"http://www.astronomynotes.com/starprop/s2.htm\" rel=\"nofollow\">http://www.astronomynotes.com/starprop/s2.htm</a>&nbsp;&nbsp;(April 23, 2008)<br /><br />1<br /><br />4<br /><br />?r2&nbsp;&nbsp;&nbsp;&nbsp;<br /><br />4?r2<br /><br /></span>",
  "pools_count": 0,
  "title": "4 wolfpup",
  "deleted": "f",
  "public": "t",
  "mimetype": "application/msword",
  "pagecount": "1",
  "rating_id": "0",
  "rating_name": "General",
  "ratings": [],
  "submission_type_id": "12",
  "type_name": "Writing - Document",
  "guest_block": "f",
  "friends_only": "f",
  "comments_count": "39",
  "views": "118"
}