|
|
테두리
|
|
 |
VhhaDGmrde |
 |
112 |
|
 |
| I'm a trainee http://xnxx.in.net/xnxxhot/ Xnxx Hot
Very long baseline interferometry has been used for about 50 years, but never before at such a high frequency, or short wavelength, of light. This short-wavelength light is what's needed to achieve the angular resolution required to measure and image black holes. |
|
 |
Arlen |
 |
2019-05-28 11:28:29 |
|
|
|
|
|
|
|
|
|
