ꯃꯔꯨꯑꯣꯏꯕ ꯂꯃꯥꯏ

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ꯃꯤꯄꯨꯝ ꯈꯨꯗꯤꯡꯃꯛ ꯁꯔꯨꯛ ꯌꯥꯕ ꯌꯥꯔꯕ ꯃꯅꯤꯡꯇꯝꯅ ꯁꯤꯖꯤꯟꯅꯕ ꯌꯥꯕ ꯃꯦꯗꯤꯌꯥ ꯐꯥꯏꯜ ১২৪,৯৭৫,১২২ꯒꯤ ꯁꯤꯡꯄꯨꯜ ꯑꯃꯅꯤ

ꯅꯨꯃꯤꯠꯁꯤꯒꯤ ꯃꯃꯤ

A close-in image of a protoplanetary disc HH 30 around a newly formed star produced by NASA/ESA/CSA James Webb Space Telescope. It is surrounded by jets and a disc wind, and is located in the dark cloud LDN 1551 in the Taurus Molecular Cloud. Herbig-Haro objects are small nebulae found in star formation regions, marking the locations where gas outflowing from young stars is heated into luminescence by shockwaves. HH 30 is an example of where this outflowing gas takes the form of a narrow jet. The source star is located on one end of the jet, hidden behind an edge-on protoplanetary disc that the star is illuminating.

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ꯅꯨꯃꯤꯠꯁꯤꯒꯤ ꯃꯦꯗꯤꯌꯥ

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ꯁꯔꯨꯛ ꯌꯥꯔꯤ

ꯊꯤꯔꯤꯔꯥ?: ꯆꯥꯟꯕꯤꯗꯨꯅ ꯂꯃꯥꯢ ꯑꯁꯤꯒꯤ ꯃꯊꯛꯇ ꯂꯩꯕ "ꯊꯤꯅꯕ ꯎꯄꯨ" ꯑꯁꯤ ꯅꯠꯇ꯭ꯔꯒ ꯌꯦꯠꯊꯪꯕꯗ ꯂꯩꯕ "ꯂꯪꯗꯥꯢ" ꯑꯁꯤ ꯁꯤꯖꯤꯟꯅꯕꯤꯌꯨ꯫ ꯑꯩꯈꯣꯢꯒꯤ ꯐꯣꯡꯗꯣꯛꯈꯤꯕ ꯄꯥꯎꯁꯤꯡ ꯑꯁꯤ ꯂꯧꯁꯤꯟꯕꯤꯕ ꯆꯤꯡꯅꯕ ꯂꯩꯕꯤꯒꯅꯨ꯫
ꯁꯤꯖꯤꯟꯅꯔꯤꯔꯥ?: ꯃꯅꯤꯡ ꯇꯝꯕ ꯆꯦ-ꯆꯥꯡ ꯒꯤ ꯑꯆꯪꯕ ꯑꯗꯨ ꯃꯄꯨꯡ ꯐꯥꯅꯅꯕ, ꯆꯥꯟꯕꯤꯗꯨꯅ ꯑꯩꯈꯣꯢꯒꯤ ꯑꯃꯨꯛ ꯍꯟꯅ ꯁꯤꯖꯤꯟꯅꯕ ꯃꯇꯦꯡ ꯑꯁꯤ ꯄꯥꯕꯤꯌꯨ꯫ ꯅꯍꯥꯛꯅ ꯃꯃꯤ ꯑꯃ ꯍꯥꯄꯤꯅꯕ ꯍꯥꯢꯖꯕ ꯑꯁꯤꯁꯨ ꯌꯥꯒꯅꯤ꯫
ꯈꯪꯗꯣꯛꯂꯤꯔꯥ?: ꯊꯤꯕꯤꯌꯨ ꯃꯆꯥꯈꯥꯢꯕ:ꯁꯛꯈꯪꯗꯕ ꯍꯤꯔꯝꯁꯤꯡꯒꯤ ꯈꯨꯠꯊꯥꯡꯗ꯫ ꯀꯔꯤꯒꯨꯝꯕ ꯅꯍꯥꯛꯅ ꯈꯪꯕ ꯉꯝꯕ ꯈꯔ ꯐꯪꯂꯕꯗꯤ, ꯄꯣꯠꯁꯛ ꯑꯗꯨꯒꯤ ꯋꯥꯔꯤ ꯁꯥꯐꯝ ꯂꯃꯥꯢ ꯗ ꯋꯥꯐꯝ ꯈꯔ ꯏꯕ ꯌꯥꯒꯅꯤ ꯫
ꯁꯦꯝꯂꯤꯔꯥ?: ꯅꯍꯥꯛꯅ ꯈꯪꯒꯗꯕ ꯂꯣꯢꯅꯃꯛ ꯑꯩꯈꯣꯢꯒꯤ ꯑꯩꯈꯣꯢꯒꯤ ꯊꯕꯛ ꯁꯔꯨꯛ ꯌꯥꯕ ꯃꯇꯦꯡ ꯑꯁꯤꯗ ꯌꯦꯡꯕꯤꯌꯨ꯫
ꯑꯗꯨꯒ ꯑꯇꯩ ꯃꯌꯥꯝ!

Discussion?: See the list of discussion pages.; ꯃꯁꯤꯒꯤ ꯊꯧꯔꯥꯡ ꯑꯁꯤꯗ ꯁꯔꯨꯛ ꯌꯥꯅꯅꯕ ꯑꯍꯦꯟꯕ ꯃꯑꯣꯡ ꯀꯌꯥ ꯈꯪꯗꯣꯛꯅꯕ ꯃꯤꯌꯥꯝꯒꯤ ꯊꯣꯡꯒꯥꯜ ꯌꯦꯡꯕꯤꯌꯨ ꯫

ꯊꯥꯒꯤ ꯑꯣꯏꯅ ꯄꯥꯡꯊꯣꯛꯄ ꯃꯤꯔꯦꯜ ꯆꯥꯡꯗꯝꯅꯕ

ꯑꯩꯈꯣꯢꯒꯤ ꯊꯥ-ꯊꯥꯒꯤ ꯑꯣꯢꯕ ꯍꯤꯔꯝ-ꯍꯤꯔꯝꯒꯤ ꯆꯥꯡꯌꯦꯡ ꯑꯁꯤ ꯊꯦꯡꯅꯕ ꯉꯝꯅꯕ ꯃꯃꯤ ꯈꯔ ꯂꯧꯕꯤꯌꯨ ꯑꯗꯨꯒ ꯊꯥꯒꯠꯄꯤꯌꯨ, ꯄꯨꯛꯅꯤꯡꯗ ꯏꯅꯣꯠ ꯄꯣꯛꯄꯤꯌꯨ ꯑꯗꯨꯒ ꯑꯅꯧꯕ ꯍꯤꯔꯝꯁꯤꯡ ꯌꯦꯡꯕꯤꯌꯨ! ꯆꯥꯡꯌꯦꯡꯁꯤꯡꯒꯤ ꯃꯇꯥꯡꯗ ꯍꯦꯟꯅ ꯈꯪꯕꯤꯌꯨ!

ꯍꯟꯗꯛꯀꯤ ꯊꯥ ꯑꯁꯤꯒꯤ ꯆꯥꯡꯌꯦꯡ ꯑꯁꯤ ꯌꯦꯡꯕꯤꯌꯨ

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