[ Supporter Features ]
[ Supporter Features ]
SteamID64: 76561198093649372
SteamID32: [U:1:133383644]
SteamID: STEAM_0:0:66691822
CommunityURL: https://steamcommunity.com/id/pandora13/
ProfileURL: https://steamcommunity.com/profiles/76561198093649372
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Status: Online
Privacy: Public
Profile Setup: True
Premium: True
Creation: 2013-06-06 04:25:52 (GMT)
Last Updated: 2024-06-24 15:45:23
VAC Banned: False
Community Banned: False
Game Banned: False
Trade Banned: False
Name | Time Changed |
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c0smicbliss | 2022-09-21 23:55:46 |
你媽媽在我床上 | 2022-09-19 07:46:32 |
MorsDeMars | 2020-05-20 07:23:46 |
Sigrun | 2020-05-19 09:02:44 |
cosmicbliss | 2020-05-14 00:14:19 |
Summerwine | 2018-08-12 06:46:20 |
Vagmuncher | 2018-08-07 23:40:03 |
Slebewww | 2018-07-09 07:27:04 |
Valkyrie | 2018-06-30 20:52:06 |
Sigrún | 2018-05-24 06:00:16 |
RealName | Time Changed |
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John Ligma | 2023-04-01 02:12:18 |
URL | Time Changed |
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https://steamcommunity.com/id/pandora13/ | 2023-04-01 02:12:18 |
State | Time Changed |
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Commenter | Message | Timestamp |
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ãlcloxa | signed by Alcloxa | 2023-09-15 14:08:24 |
Satan | Arthur Morgan stands at 6'1, weighs 185lbs, and is of a muscular build. He has dark blonde hair and bluish green eyes. His body type can be affected by the player's eating habits as well. Over indulging in food will make him appear fatter, and will increase his health while lowering his stamina, and not eating enough will make him slimmer, Increasing his speed while lowering his health.The player can determine what he looks like. He can either be messy, clean, or a little bit of both. He can have a beard or not depending if the player decides to let his beard grow or shave it. He can either have long hair or short hair as well, again, depending on how the player treats him. After beating up a man named Thomas Downes, he contracted Tuberculosis, which makes him appear slightly pale with his eyes looking sickly. He can also have red cheeks, well red. | 2022-09-19 08:04:15 |
Satan | A black hole is a region of spacetime where gravity is so strong that nothing—no particles or even electromagnetic radiation such as light—can escape from it.[1] The theory of general relativity predicts that a sufficiently compact mass can deform spacetime to form a black hole.[2][3] The boundary of no escape is called the event horizon. Although it has an enormous effect on the fate and circumstances of an object crossing it, according to general relativity it has no locally detectable features.[4] In many ways, a black hole acts like an ideal black body, as it reflects no light.[5][6] Moreover, quantum field theory in curved spacetime predicts that event horizons emit Hawking radiation, with the same spectrum as a black body of a temperature inversely proportional to its mass. This temperature is on the order of billionths of a kelvin for black holes of stellar mass, making it essentially impossible to observe directly. | 2021-10-08 21:03:45 |
Shower | https://twitter.com/dailypornvidzzz/status/1438992994858778630?s=20https://twitter.com/dailypornvidzzz/status/1438992994858778630?s=20https://twitter.com/dailypornvidzzz/status/1438992994858778630?s=20https://twitter.com/dailypornvidzzz/status/1438992994858778630?s=20https://twitter.com/dailypornvidzzz/status/1438992994858778630?s=20https://twitter.com/dailypornvidzzz/status/1438992994858778630?s=20 | 2021-09-20 09:30:33 |
Shower | https://twitter.com/dailypornvidzzz/status/1438992994858778630?s=20 | 2021-09-20 09:30:21 |
Shower | https://twitter.com/dailypornvidzzz/status/1438992994858778630?s=20 | 2021-09-20 09:30:18 |
Shower | The black hole area theorem, which Hawking derived in 1971 from Einstein's theory of general relativity, states that it is impossible for the surface area of a black hole to decrease over time. This rule interests physicists because it is closely related to another rule that appears to set time to run in a particular direction: the second law of thermodynamics, which states that the entropy, or disorder, of a closed system must always increase. Because a black hole's entropy is proportional to its surface area, both must always increase.According to the new study, the researchers' confirmation of the area law seems to imply that the properties of black holes are significant clues to the hidden laws that govern the universe. Oddly, the area law seems to contradict another of the famous physicist's proven theorems: that black holes should evaporate over extremely long time scale, so figuring out the source of the contradiction between the two theories could reveal new physics. | 2021-09-20 02:25:25 |
Shower | The black hole area theorem, which Hawking derived in 1971 from Einstein's theory of general relativity, states that it is impossible for the surface area of a black hole to decrease over time. This rule interests physicists because it is closely related to another rule that appears to set time to run in a particular direction: the second law of thermodynamics, which states that the entropy, or disorder, of a closed system must always increase. Because a black hole's entropy is proportional to its surface area, both must always increase.According to the new study, the researchers' confirmation of the area law seems to imply that the properties of black holes are significant clues to the hidden laws that govern the universe. Oddly, the area law seems to contradict another of the famous physicist's proven theorems: that black holes should evaporate over extremely long time scale, so figuring out the source of the contradiction between the two theories could reveal new physics. | 2021-09-20 02:24:42 |
Shower | The black hole area theorem, which Hawking derived in 1971 from Einstein's theory of general relativity, states that it is impossible for the surface area of a black hole to decrease over time. This rule interests physicists because it is closely related to another rule that appears to set time to run in a particular direction: the second law of thermodynamics, which states that the entropy, or disorder, of a closed system must always increase. Because a black hole's entropy is proportional to its surface area, both must always increase.According to the new study, the researchers' confirmation of the area law seems to imply that the properties of black holes are significant clues to the hidden laws that govern the universe. Oddly, the area law seems to contradict another of the famous physicist's proven theorems: that black holes should evaporate over extremely long time scale, so figuring out the source of the contradiction between the two theories could reveal new physics. | 2021-09-20 02:24:39 |
Shower | The black hole area theorem, which Hawking derived in 1971 from Einstein's theory of general relativity, states that it is impossible for the surface area of a black hole to decrease over time. This rule interests physicists because it is closely related to another rule that appears to set time to run in a particular direction: the second law of thermodynamics, which states that the entropy, or disorder, of a closed system must always increase. Because a black hole's entropy is proportional to its surface area, both must always increase.According to the new study, the researchers' confirmation of the area law seems to imply that the properties of black holes are significant clues to the hidden laws that govern the universe. Oddly, the area law seems to contradict another of the famous physicist's proven theorems: that black holes should evaporate over extremely long time scale, so figuring out the source of the contradiction between the two theories could reveal new physics. | 2021-09-20 02:24:36 |
Demon | panik ga? | 2021-08-24 21:26:02 |
Jamur Krispi | Gendut | 2020-12-01 08:40:14 |
21 | roseau | 2017-07-06 18:18:40 |
set | close | 2017-04-27 22:45:15 |
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