资讯
The Brighterside of News on MSN1 天
Astronomers found the building blocks of new planets swirling around two young stars
Astronomers have discovered the raw ingredients of planets orbiting two infant stars, offering a glimpse into how new worlds ...
11 天
The Brighterside of News on MSNSwirling clouds of gas and dust rich in CO2, not water form planets, study finds
In the swirling clouds of gas and dust that surround newborn stars, planets begin to form. These planet-forming disks are ...
Astronomers using ALMA have discovered that planet-forming discs are not flat and serene but subtly warped, reshaping our ...
Interstellar objects like 3I/ATLAS that have been captured in planet-forming discs around young stars could become the seeds ...
1 小时
The Brighterside of News on MSNCosmic warps could be the missing key to planet formation
The long-standing idea of planets forming in perfectly flat, orderly discs has been challenged by new research. Instead of ...
Planets may begin forming much earlier than scientists once believed during the final stages of a star s birth, not afterward. This bold new model, backed by simulations from researchers at SwRI, ...
Pictures are the key to new insights in the field of astrophysics. Such images include simulations of cosmic events, which astrophysicists at UZH use to investigate how stars, planets and galaxies ...
Archival ALMA data revealed a large, expanding bubble near the protoplanetary disk of the young star WSB 52, located approximately 441 light-years away. The bubble's formation is hypothesized to ...
Pictures are the key to new insights in the field of astrophysics. Such images include simulations of cosmic events, which astrophysicists at UZH use to investigate how stars, planets and galaxies ...
Cecilia Payne-Gaposchkin discovered the composition of stars at the age of 25: hydrogen, helium, and traces of nearly all other elements. Her 1925 discovery was one of the earliest successful attempts ...
Cecilia Payne-Gaposchkin discovered the composition of stars at the age of 25: hydrogen, helium, and trace amounts of almost all other elements. Her discovery in 1925 was one of the earliest attempts ...
一些您可能无法访问的结果已被隐去。
显示无法访问的结果