c0smicbliss
John Ligma
 
 
白鳥は
哀しからずや
空の青
海のあをにも
染まずただよふ
若山牧水
Şu Anda Çevrimiçi
Ekran Görüntüsü Vitrini
Favori Oyun
İnceleme Vitrini
228 saat oynandı
praise the but hole
İnceleme Vitrini
122 saat oynandı
Nice 10/10
Son Etkinlikler
kayıtlarda 32 saat
son oynanma: 17 Ara
kayıtlarda 30 saat
son oynanma: 17 Ara
kayıtlarda 110 saat
son oynanma: 16 Ara
ãlcloxa 15 Eyl 2023 @ 12:08 
signed by Alcloxa
Satan 19 Eyl 2022 @ 6:04 
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.
Satan 8 Eki 2021 @ 19:03 
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.