利用微小宇宙尘埃粒子云进行评估

Rahmatullah Lewal, Sherwali Hemat
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引用次数: 0

摘要

我们在这篇文章中谈到了宇宙尘埃粒子的存在,它们由不同的元素组成,如碳、氧、铁以及其他比氢和氦重的原子。恒星的形成有赖于宇宙尘埃粒子,它们是行星和人类的组成部分。落到地球上或存在于太空中的尘埃被称为宇宙尘埃,有时也被称为地外尘埃或太空尘埃。大多数宇宙尘埃粒子的大小在几个分子到 0.1 毫米(100 微米)之间。我们把较大的颗粒称为陨石。宇宙尘埃被认为是小行星或彗星碰撞的残留物,与宇宙大爆炸期间发生的碰撞有关。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Evaluations Using Clouds of Tiny Cosmic Dust Particles
We talked about the existence of cosmic dust particles in this article, which are composed of different elements like carbon, oxygen, iron, and other atoms heavier than hydrogen and helium. Star formation depends on cosmic dust particles, which are the building blocks of planets and people. Dust that has fallen to Earth or exists in space is known as cosmic dust, sometimes known as extraterrestrial dust or space dust. The majority of particles of cosmic dust have sizes between a few molecules and 0.1 mm (100 µm). We refer to larger particles as meteorites. Cosmic dust is thought to be the remnants of asteroidal or cometary collisions that can be linked to collisions that took place during the Big Bang.
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