{"id":5577,"date":"2017-01-18T17:38:22","date_gmt":"2017-01-18T16:38:22","guid":{"rendered":"http:\/\/reperes-astro.fr\/?p=5577"},"modified":"2025-01-20T15:38:57","modified_gmt":"2025-01-20T14:38:57","slug":"ic-410-par-mathieu","status":"publish","type":"post","link":"https:\/\/reperes-astro.fr\/ic-410-par-mathieu\/","title":{"rendered":"Derni\u00e8res productions de Mathieu"},"content":{"rendered":"\n

VOIR LE SITE DE MATHIEU ICI<\/a>.<\/strong><\/p>\n\n\n\n

IC410<\/strong><\/h2>\n\n\n
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IC 410<\/figcaption><\/figure>\n<\/div>\n\n\n

Camera CCD QSI 683ws8 sur lunette Televue 101\/540 et Eq6 pro goto.<\/p>\n\n\n\n

(Echantillonage 2.06 arcsec\/pixel)<\/p>\n\n\n\n

Auto guidage diviseur optique + zwo Asi 120mm<\/p>\n\n\n\n

14 heures de poses les 26 et 28 d\u00e9cembre 2016 et 2 janvier 2017.<\/p>\n\n\n\n

\u200bH : 46*10 mn bin1<\/p>\n\n\n\n

O : 40*5 mn bin2<\/p>\n\n\n\n

S : 36*5 mn bin2<\/p>\n\n\n\n

\u200bTraitement Prism v9, Pixinsight, Photoshop<\/p>\n\n\n\n

\u00a0M 42 LA NEBULEUSE D’ORION<\/strong><\/h2>\n\n\n
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M42<\/figcaption><\/figure>\n<\/div>\n\n\n

\u00a0Camera CCD QSI 683ws8 sur lunette Televue 101\/540 et Eq6 pro goto.<\/p>\n\n\n\n

(Echantillonage 2.06 arcsec\/pixel)<\/p>\n\n\n\n

Auto guidage diviseur optique + zwo Asi 120mm<\/p>\n\n\n\n

3h30 de poses en janvier 2017.<\/p>\n\n\n\n

\u200bH : 12*10 mn bin1<\/p>\n\n\n\n

R : 6*5 mn bin2<\/p>\n\n\n\n

V : 6*5 mn bin2<\/p>\n\n\n\n

B : 6*5mn bin2<\/p>\n\n\n\n

\u200b+ poses de 30 secondes HRVB pour le coeur de la n\u00e9buleuse fort brillant<\/p>\n\n\n\n

\u200bTraitement Prism v9, Pixinsight, Photoshop HRVB<\/p>\n\n\n\n

\u00a0La n\u00e9buleuse d’Orion ou M42<\/strong> est une n\u00e9buleuse en \u00e9mission\/r\u00e9flexion situ\u00e9e dans la constellation du m\u00eame nom.<\/span><\/p>\n\n\n\n

Sur cette image \u00e9galement M43 et NGC 1977, appel\u00e9e aussi Running man nebula.<\/span><\/p>\n\n\n\n

Elle est la n\u00e9buleuse diffuse<\/span><\/a> la plus luisante, visible \u00e0 l’\u0153il nu dans un ciel de nuit sans pollution lumineuse<\/span><\/a> et peut \u00eatre facilement vue avec des jumelles<\/span><\/a>. Elle se r\u00e9pand sur un pan de ciel de 66 \u00d7 60 minutes d’arc<\/span><\/a>, soit quatre fois plus que la pleine lune<\/span><\/a>. La n\u00e9buleuse a une taille d’environ 33 ann\u00e9es-lumi\u00e8re.<\/span><\/p>\n\n\n\n

Il aura fallu attendre 2007 pour s’apercevoir que la n\u00e9buleuse se trouve \u00e0 environ 1 350 ann\u00e9es-lumi\u00e8re<\/span><\/a> de la Terre<\/span><\/a> au lieu des 1 500 ann\u00e9es-lumi\u00e8re<\/span><\/a> jusque-l\u00e0 estim\u00e9es. Elle contient un amas ouvert<\/span><\/a> tr\u00e8s jeune renfermant de nombreuses \u00e9toiles<\/span><\/a>. (wiki)<\/em><\/span><\/p>\n\n\n\n

M45 LES PLEIADES<\/strong><\/h2>\n\n\n
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LES PLEIADES<\/figcaption><\/figure>\n<\/div>\n\n\n

\u00a0Lunette Televue 101\/540 Genesis sdf et camera QSI 683 ws8<\/p>\n\n\n\n

7h50 de poses les 31 octobre, 2, 21, 28 novembre et 3 d\u00e9cembre 2016 \u00e0 Amiens.<\/p>\n\n\n\n

L : 21*10 mn bin1<\/p>\n\n\n\n

R : 6 * 10mn bin2<\/p>\n\n\n\n

G : 10*10mn bin2<\/p>\n\n\n\n

B : 10*10mn bin2<\/p>\n\n\n\n

\u200bTraitement Prism, Pixinsight, Photoshop.<\/p>\n\n\n\n

Les Pl\u00e9iades, ou M45<\/strong>, sont un amas ouvert<\/span><\/a> d’\u00e9toiles qui s’observe dans l’h\u00e9misph\u00e8re nord, dans la constellation du Taureau<\/span><\/a>.<\/span><\/p>\n\n\n\n

Il existe un d\u00e9bat concernant l’exactitude de la distance de l’amas \u00e0 la Terre. Cette distance, selon les diff\u00e9rents instruments techniques utilis\u00e9s, pourrait \u00eatre estim\u00e9e \u00e0 environ 444 ann\u00e9es-lumi\u00e8re.<\/span><\/p>\n\n\n\n

On d\u00e9nombre aujourd’hui dans cet amas environ 3 000 \u00e9toiles<\/span><\/a>, dont une douzaine sont visibles \u00e0 l’\u0153il nu. Il s’\u00e9tend sur 2\u00b0, soit l’\u00e9quivalent de quatre fois le diam\u00e8tre apparent de la Lune<\/span><\/a>. Sa densit\u00e9 est donc relativement faible par rapport aux autres amas ouverts. L’\u00e2ge de l’amas est estim\u00e9 \u00e0 100 millions d’ann\u00e9es, mais il ne devrait pas vivre longtemps puisqu’il devrait se s\u00e9parer dans 250 millions d’ann\u00e9es, en partie \u00e0 cause de sa faible densit\u00e9 (il s’agit ici de la vie de l’amas et non de celle des \u00e9toiles qui le composent).<\/span><\/p>\n\n\n\n

Les 9 \u00e9toiles les plus brillantes de l’amas tirent leur nom des pl\u00e9iades (7 s\u0153urs) et de leurs parents. Leur magnitude apparente<\/span><\/a> est comprise entre +2,86 et +5,44, donc accessible \u00e0 l’\u0153il nu. Ast\u00e9rope<\/span><\/a> a la particularit\u00e9 d’\u00eatre une \u00e9toile double. (wikipedia)<\/em><\/span><\/p>\n\n\n\n

Les n\u00e9buleuses par r\u00e9flexion<\/span><\/a> sont le reflet de la lumi\u00e8re d’une \u00e9toile proche sur d’innombrables petits grains de carbone<\/span><\/a>. La couleur bleue des n\u00e9buleuses par r\u00e9flexion<\/span><\/a> vient du fait que la partie bleue du spectre lumineux est plus efficacement diffus\u00e9e<\/span><\/a> par la poussi\u00e8re<\/span><\/a> de carbone que la partie rouge. L’\u00e9clat de la n\u00e9buleuse<\/span><\/a> est quant \u00e0 lui d\u00e9termin\u00e9 par la taille et la densit\u00e9 des grains r\u00e9fl\u00e9chissants, et bien s\u00fbr par la couleur et l’intensit\u00e9 du rayonnement de l’\u00e9toile, source primaire de lumi\u00e8re.<\/span><\/p>\n\n\n\n

La n\u00e9bulosit\u00e9 dans laquelle baignent les Pl\u00e9iades<\/span><\/a> n’est pas comme on l’a longtemps cru un vestige du nuage dans lequel elles se sont form\u00e9es, mais est en fait due \u00e0 une rencontre fortuite<\/span><\/a> entre l’amas ouvert<\/span><\/a> et un nuage mol\u00e9culaire<\/span><\/a> de poussi\u00e8res.<\/span><\/p>\n\n\n\n

<\/p>\n

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VOIR LE SITE DE MATHIEU ICI. IC410 Camera CCD QSI 683ws8 sur lunette Televue 101\/540 et Eq6 pro goto. (Echantillonage 2.06...<\/p>\n

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<\/div>\n","protected":false},"author":2,"featured_media":5575,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[108,102,72],"tags":[],"class_list":["post-5577","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-archives-reperes-astro-2017","category-archives-reperes-astro","category-astrophotos-reperes-astro"],"yoast_head":"Derni\u00e8res productions de Mathieu - Rep\u00e8res Astro<\/title>\n<meta name=\"robots\" content=\"index, follow, max-snippet:-1, max-image-preview:large, max-video-preview:-1\" \/>\n<link rel=\"canonical\" href=\"https:\/\/reperes-astro.fr\/ic-410-par-mathieu\/\" \/>\n<meta property=\"og:locale\" content=\"fr_FR\" \/>\n<meta property=\"og:type\" content=\"article\" \/>\n<meta property=\"og:title\" content=\"Derni\u00e8res productions de Mathieu - Rep\u00e8res Astro\" \/>\n<meta property=\"og:description\" content=\"VOIR LE SITE DE MATHIEU ICI. 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