Научно-популярный информационный портал

Тег: космос

Составлена карта быстрых облаков нашей Галактики

экзопланета HD 189733b планета космос

Жизнь на планетах может быть не видна из-за атмосферы

Учёные поняли, почему Плутон холоднее, чем нужно

Астрономы определили ближайшую к Солнечной системе планету для возможного заселения

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.

Учёные смоделировали загадочное столкновение двух нейтронных звёзд

Спутник. Или «запуск» космической эры

Учёные открыли экзопланету, опровергающую теорию происхождения небесных тел

Сияния на полюсах Сатурна не связаны друг с другом

свет космос рука вселенная муть хрень

Учёные попытались объяснить трёхмерность Вселенной

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.

Учёные впервые зарегистрировали гравитационные волны от слияния нейтронных звёзд