MXB 1658-298

作者: SevenSpheres Cham Vision

公開日:

MXB 1658-298, also known as V2134 Ophiuchi, is a distant X-ray binary star system consisting of a pulsar and a K-type main sequence star about 32,615 light-years away in the constellation Ophiuchus. In 2017, a massive substellar companion about 23 times the mass of Jupiter was detected via eclipse timing variations, completing a single orbit around both stars once every 2.1 years

このページの翻訳に こちらから ご協力ください。

Celestia で開く（推奨） または ダウンロード

アドオンのインストール方法は？ こちら をご覧ください。