You'll be getting 38 graphics (coloured and lineart) that explains kinetic theory of matterExperiments Illustrations:Diffusion in Solids, Liquids and GasesEffect of Molecular Mass on DiffusionDiffusion through BalloonKinetic Particle Theory:Solid, Liquid and Gases (2D)Solid, Liquid and Gases (3D)Brownian MotionWaterIceSteamThis is part of a Matter Clipart Bundle that contains the following sets:1) Kinetic Theory of Matter (Solids, Liquids, Gases)2) Elements, Compounds and Mixtures3) Metals…
A molecular cloud near IRAS 14568-6304. Credit (NASA/ESA/Luca Limatola) For more information about #Giant #Molecular #Clouds check out: http://astronomyisawesome.com/universe/giant-molecular-clouds-the-stellar-nursery/
A photogenic group of nebulae can be found in Chamaeleon, a constellation visible predominantly in skies south of the Earth's equator. Towards Chamaeleon, dark molecular clouds and bright planetary nebula NGC 3195 can be found. Visible near the center of the above photograph is a reflection nebula surrounding a young bright star. On the lower right, a dark molecular cloud blocks the light from stars behind it.
Stars ~ Stars form in the densest regions of the interstellar medium, or ISM, called molecular clouds. The ISM is the name given to the gas and dust that exists between the stars within a galaxy. It is 99% gas and 1% dust, by mass. Molecular clouds are perfect star-forming regions because the combination of these atoms into molecules is much more likely in very dense regions.
#SolarSystem facts : The Solar System consists of the #Sun and the astronomical objects gravitationally bound in orbit around it, all of which formed from the collapse of a giant molecular cloud approximately 4.6 billion years ago. 99.86% of the system’s mass is in the Sun.