Exif II*
f n ( 1 v 2 ; ! i Artist concept of the so-called "snow line" in the young planet-forming system known as TW Hydrae. A snow line is where particles become icy and can more easily stick together to make larger chunks when they collide. This is one way for planets to form. ALMA has found water-covered ice grains in this system's inner disk (4.5 -- 30 AU, blue) and carbon monoxide (CO) ice-covered grains in the outer disk (>30 AU, green). The transition from blue to green marks the CO snow line. - ' - ' Adobe Photoshop CS6 (Macintosh) 2017-02-10T13:58:14-05:00 NRAO/AUI/NSF https://public.nrao.edu/mediause 0220 *http://ns.adobe.com/xap/1.0/ NRAO/AUI/NSF https://public.nrao.edu/mediause Finding Ice in Baby Solar Systems Artist concept of the so-called \"snow line\" in the young planet-forming system known as TW Hydrae. A snow line is where particles become icy and can more easily stick together to make larger chunks when they collide. This is one way for planets to form. ALMA has found water-covered ice grains in this system\'s inner disk (4.5 -- 30 AU, blue) and carbon monoxide (CO) ice-covered grains in the outer disk (>30 AU, green). The transition from blue to green marks the CO snow line. TW Hydrae 0644E1894C6C5CE2F6A2FC01C7AB000A 4475164089CBA86E05A91F0621E49334 4A3BA6AE185FFC62FF52E607A7EA8857 AA5995C473AD6DE6CC91586371B6BFB6 adobe:docid:photoshop:53418ab9-51b5-11d9-8fe4-fbd02b7f9b17 adobe:docid:photoshop:6f778eb1-4b57-11d9-936f-b3e4249ab0f0 uuid:0A996126206DDC118021A7CAE2820A99 Creative Commons Attribution 3.0 Unported license (http://creativecommons.org/licenses/by/3.0/) B.3.7.2.1 176 Alexandra Angelich and Bill Saxton (NRAO/AUI/NSF)http://epocms-alpha.nrao.edu/wp-content/uploads/2017/01/TWHydrae_Snowline.jpghttps://public.nrao.edu/gallery/finding-ice-in-baby-solar-systems-2/ *http://ns.adobe.com/xap/1.0/ NRAO/AUI/NSF https://public.nrao.edu/mediause Finding Ice in Baby Solar Systems Artist concept of the so-called \"snow line\" in the young planet-forming system known as TW Hydrae. A snow line is where particles become icy and can more easily stick together to make larger chunks when they collide. This is one way for planets to form. ALMA has found water-covered ice grains in this system\'s inner disk (4.5 -- 30 AU, blue) and carbon monoxide (CO) ice-covered grains in the outer disk (>30 AU, green). The transition from blue to green marks the CO snow line. TW Hydrae 0644E1894C6C5CE2F6A2FC01C7AB000A 4475164089CBA86E05A91F0621E49334 4A3BA6AE185FFC62FF52E607A7EA8857 AA5995C473AD6DE6CC91586371B6BFB6 adobe:docid:photoshop:53418ab9-51b5-11d9-8fe4-fbd02b7f9b17 adobe:docid:photoshop:6f778eb1-4b57-11d9-936f-b3e4249ab0f0 uuid:0A996126206DDC118021A7CAE2820A99 Creative Commons Attribution 3.0 Unported license (http://creativecommons.org/licenses/by/3.0/) B.3.7.2.1 176 Alexandra Angelich and Bill Saxton (NRAO/AUI/NSF)http://epocms-alpha.nrao.edu/wp-content/uploads/2017/01/TWHydrae_Snowline.jpghttps://public.nrao.edu/gallery/finding-ice-in-baby-solar-systems-2/ Photoshop 3.0 8BIM Z %G xArtist concept of the so-called "snow line" in the young planet-forming system known as TW Hydrae. A snow line is where particles become icy and can more easily stick together to make larger chunks when they collide. This is one way for planets to form. ALMA has found water-covered ice grains in this system's inner disk (4.5 -- 30 AU, blue) and carbon monoxide (CO) ice-covered grains in the outer disk (>30 AU, green). The transition from blue to green marks the CO snow line.i !Finding Ice in Baby Solar SystemsP NRAO/AUI/NSFn Alexandra Angelich and Bill Saxts NRAO/AUI/NSF !Finding Ice in Baby Solar Systems TW Hydraet https://public.nrao.edu/mediause 8BIM% C
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