Astronomy Picture of the Day Discover the cosmos!Each day a different image or photograph of our fascinating universe is featured, along with a brief explanation written by a professional astronomer.2024 December 22 The Local Fluff Illustration Credit: NASA, SVS,Adler, U. Chicago, Wesleyan Explanation: The stars are not alone. In the disk of ourMilky Way Galaxy,about 10 percent of visible matter is in the form of gas called theinterstellar medium (ISM). The ISM isnot uniformand shows patchiness even near ourSun. It can be quite difficult to detect thelocal ISM because it is so tenuous and emits so little light. This mostly hydrogen gas, however, absorbs some veryspecific colors that can be detected in the light of thenearest stars. A working map of the localISM within 20 light-years,based on ongoing observations and particle detections from the Earth-orbiting Interstellar Boundary Exporer satellite (IBEX), is shown here. These observations indicate that ourSun is moving through aLocal Interstellar Cloud as this cloud flows outwards from theScorpius-Centaurus Association star forming region. Our Sun may exit the Local Cloud, also called the Local Fluff, during the next 10,000 years. Much remains unknown about the localISM, including details of its distribution,its origin, and how it affects theSun and the Earth.Unexpectedly, IBEXspacecraft measurements indicate that the direction from which neutral interstellar particles flow through our Solar System is changing. APOD Year in Review: Night Sky Network Presentation for 2024 Tomorrow's picture: sky tree <| Archive| Submissions | Index| Search| Calendar| RSS| Education| About APOD| Discuss| > Authors & editors: Robert Nemiroff(MTU) &Jerry Bonnell (UMCP)NASA Official: Amber StraughnSpecific rights apply.NASA Web Privacy,Accessibility, Notices; A service of:ASD atNASA /GSFC, NASA Science Activation& Michigan Tech. U.