1Our GalaxyChapter Twenty-FiveGuiding Questions1. What is our Galaxy? How do astronomers know where we are located within it?2. What is the shape and size of our Galaxy?3. How do we know that our Galaxy has spiral arms?4. What is most of the Galaxy made of? Is it stars, gas, dust, or something else?5. What is the nature of the spiral arms?6. What lies at the very center of our Galaxy?Interstellar dust obscures our view at visible wavelengths along lines of sight that lie in the plane of the galactic disk2As a result, the Sun’s location in the Galaxy was unknown for many yearsThis dilemma was resolved by observing parts of the Galaxy outside the disk3Determining the distance and direction of the globular clusters gave us the Sun’s locationOur Sun lies within the galactic disk, some 8000 pc (26,000 ly) from the center of the GalaxyObservations at nonvisible wavelengths revealthe shape of the Galaxy4There are about 200 billion (2 × 1011) stars in the Galaxy• Our Galaxy has a disk about 50 kpc (160,000 ly) in diameter and about 600 pc (2000 ly) thick, with a high concentration of interstellar dust and gas in the disk• The Sun orbits around the center of the Galaxy at a speed of about 790,000 km/h• It takes about 220 million years to complete one orbit• The galactic center is surrounded by a large distribution of stars called the central bulge• This bulge is not perfectly symmetrical, but may have a bar or peanut shape• The disk of the Galaxy is surrounded by a spherical distribution of globular clusters and old stars, called the galactic haloThe spin-flip transition in hydrogen emits 21-cm radio waves5• This is the same physical principle behind magnetic resonance imaging (MRI),an important diagnostic tool of modern medicineThese emissions easily penetrate the intervening interstellar dustSpiral arms can be traced from the positions of clouds of atomic hydrogen6OB associations, H II regions, and molecular clouds in the galactic disk outline huge spiral arms7The rotation of our Galaxy reveals the presenceof dark matterFrom studies of the rotation of the Galaxy, astronomers estimate that the total mass of the Galaxy is about 1012M89Only about 10% of this mass is in the form of visible stars, gas, and dust• The remaining 90% is in some nonvisible form, called dark matter, that extends beyond the edge of the luminous material in the Galaxy• Our Galaxy’s dark matter may be a combination of MACHOs (dim, star-sized objects), massive neutrinos, and WIMPs (relatively massive subatomic particles)Spiral arms are caused by density waves that sweep around the Galaxy• There are two leading theories of spiral structure in galaxies• According to the density-wave theory, spiral arms are created by density waves that sweep around the Galaxy• The gravitational field of this spiral pattern compresses the interstellar clouds through which it passes, thereby triggering the formation of the OB associations and H II regions that illuminate the spiral arms1011• According to the theory of self-propagating star formation, spiral arms are caused by the birth of stars over an extended region in a galaxy• Differential rotation of the galaxy stretches the starforming region into an elongated arch of stars and nebulae.12The innermost part of the Galaxy, or galactic nucleus, has been studied through its radio, infrared, and X-ray emissions (which are able to pass through interstellar dust)13A strong radio source called Sagittarius A* is located at the galactic centerThis marks the position of a supermassive black hole with a mass of about 3.7 × 106M14Key Words• central bulge (of a galaxy)• dark matter• density wave• disk (of a galaxy)• far-infrared• flocculent spiral galaxy• galactic nucleus•galaxy• globular cluster• grand-design spiral galaxy•H I• halo (of a galaxy)• high-velocity star• interstellar extinction• Local Bubble• magnetic resonance imaging (MRI)• massive compact halo object (MACHO)• microlensing•Milky Way Galaxy• near-infrared• rotation curve• RR Lyrae variable• Sagittarius A*• self-propagating star formation• spin (of a particle)• spin-flip transition• spiral arm• 21-cm radio emission• weakly interacting massive particle (WIMP)• winding
View Full Document
Unlocking...