From: owner-ammf-digest@smoe.org (alt.music.moxy-fruvous digest) To: ammf-digest@smoe.org Subject: alt.music.moxy-fruvous digest V14 #14476 Reply-To: ammf@fruvous.com Sender: owner-ammf-digest@smoe.org Errors-To: owner-ammf-digest@smoe.org Precedence: bulk alt.music.moxy-fruvous digest Sunday, August 18 2024 Volume 14 : Number 14476 Today's Subjects: ----------------- Odd Little Device Trumps Solar Panels in the Eyes of Americans ["Trumps S] ---------------------------------------------------------------------- Date: Sun, 18 Aug 2024 09:41:45 +0200 From: "Trumps Solar Panels" Subject: Odd Little Device Trumps Solar Panels in the Eyes of Americans Odd Little Device Trumps Solar Panels in the Eyes of Americans http://tribalamp.shop/203X_x0anGIFKNdK6xdp8CGvNLuyHb6LiblrFct1jDBnENxZpw http://tribalamp.shop/vSLaMQfGC574Xj6uES6djvuFwpN1uUATYX2xYp3q44ux4U2yQw ach one is loosely bound by mutual gravitational attraction and becomes disrupted by close encounters with other clusters and clouds of gas as they orbit the Galactic Center. This can result in a loss of cluster members through internal close encounters and a dispersion into the main body of the galaxy. Open clusters generally survive for a few hundred million years, with the most massive ones surviving for a few billion years. In contrast, the more massive globular clusters of stars exert a stronger gravitational attraction on their members, and can survive for longer. Open clusters have been found only in spiral and irregular galaxies, in which active star formation is occurring. Young open clusters may be contained within the molecular cloud from which they formed, illuminating it to create an H II region. Over time, radiation pressure from the cluster will disperse the molecular cloud. Typically, about 10% of the mass of a gas cloud will coalesce into stars before radiation pressure drives the rest of the gas away. Open clusters are key objects in the study of stellar evolution. Because the cluster members are of similar age and chemical composition, their properties (such as distance, age, metallicity, extinction, and velocity) are more easily determined than they are for isolated stars. A number of open clusters, such as the Pleiades, the Hyades and the Alpha Persei Cluster, are visible with the naked eye. Some others, such as the Double Cluster, are barely perceptible without instruments, while many more can be s ------------------------------ End of alt.music.moxy-fruvous digest V14 #14476 ***********************************************