Научно-популярный информационный портал

Тег: астрономия

Млечный путь космос

Найден новый вид гигантских туманностей

Нейросеть нашла 301 новую экзопланету

На Марсе снова нашли органику

Mars surface close to equator

Израиль Марстағы өмірге еліктей бастады

В Израиле начали имитировать жизнь на Марсе

Ауыр нейтрондық жұлдыздар қалай алынады

Chandra data (above, graph) on J0806 show that its X-rays vary with a period of 321.5 seconds, or slightly more than five minutes. This implies that the X-ray source is a binary star system where two white dwarf stars are orbiting each other (above, illustration) only 50,000 miles apart, making it one of the smallest known binary orbits in the Galaxy. According to Einstein's General Theory of Relativity, such a system should produce gravitational waves - ripples in space-time - that carry energy away from the system and cause the stars to move closer together. X-ray and optical observations indicate that the orbital period of this system is decreasing by 1.2 milliseconds every year, which means that the stars are moving closer at a rate of 2 feet per year.

Как получаются тяжёлые нейтронные звёзды

космос галактика андромеда

Космический пейзаж превратили в музыку

Mars surface close to equator

Космическая стройка: изобретён заменитель бетона на моче и крови

Почему у астероидов Бенну и Рюгу странная форма