An observation made by NASA’s SPHEREx (Spectro-Photometer for the History of the Universe, Epoch of Reionization, and Ices Explorer) shows the chemical signatures of water ice (shown in bright blue) and polycyclic aromatic hydrocarbons (orange) in Cygnus X, one of the most active and turbulent regions of star birth in our Milky Way galaxy.
Category:
Photojournal, SPHEREx (Spectro-Photometer for the History of the Universe and Ices Explorer)
Posted on
April 15, 2026
Sign up for our newsletter:
Categories
5
124
1
6
1
8
18
11
1
155
5
2
1
10
226
10
2
10
10
1
10
1
2
149
10
3
41
1
2
1
8
20
14
3
14
1
30
2
214
45
2
17
1
4
640
1
10
1
2
1
1
377
37
14
26
2
18
1
47
2
296
42
44
1
1
7
7
6
3
1
29
10
17
5
17
33
6
1
16
39
134
1
1
203
1
3
10
1
198
1
105
104
353
1
10
1
68
2
51
10
6
1
3
1
3
1
2
44
4
1
137
21
1
93
2
2
110
13
2
11
10
2
1
4
18
163
2
1
29
1
5
11
21
3
55
1
13
108
14
395
6
1
33
6
62
33
26
14
38
3
1
180
4
3
25
2
18
17
2
3
110
3
13
4
4
1
1
13
6
1
373
48
15
1
12
57
34
1
5
35
5
1
360
2
12
1
271
Blog Posts
2026 IGARSS Hyperwall Schedule
August 7, 2026
NASA’s IXPE Studies Magnetar
August 7, 2026