science vpcab mr albert River

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Across
  1. 4. The upper boundary to the mass of a white dwarf.
  2. 8. An object, midway in size between a planet and a star, with a mass about 1/100 that of the sun.
  3. 10. A measure of the observed light received from a star or other object.
  4. 13. The central part of a galaxy.
  5. 15. A morphological classification scheme for galaxies. Often described as a tuning fork, after the shape of the diagram created from it.
  6. 16. A large assemblage of stars, gas, dust, and dark matter orbiting a common center.
  7. 17. A star that experiences a sudden outburst of radiant energy, temporarily exponentially increasing its luminosity.
  8. 18. A theoretical point of zero volume and infinite density to which any black hole must collapse.
  9. 20. The distance from the center of a black hole to its event horizon.
  10. 22. A cloud of interstellar gas or dust.
  11. 23. An assemblage of stars, oval in shape, that contains no conspicuous interstellar material.
  12. 24. A low-mass star that has exhausted most or all of its nuclear fuel and has collapsed to a very small size.
  13. 25. The classification of stars according to their temperatures using the characteristics of their spectra.
  14. 26. Large, cold, interstellar clouds with large diameters where massive stars form.
  15. 27. A star of very high luminosity and relatively low temperature.
  16. 29. A flattened, rotating, large assemblage of stars with pinwheel-like arms of interstellar material and stars winding out from its nucleus.
  17. 32. A spherical collection of stars that orbits a galactic core as a satellite.
  18. 33. The surface at which the escape velocity of a collapsing star is equal to the speed of light.
  19. 34. An explosion that marks the final stage of stellar evolution.
  20. 35. A collapsed, massive body whose escape velocity is equal to or greater than the speed of light.
Down
  1. 1. A star of extremely high density composed almost entirely of neutrally charged subatomic particles.
  2. 2. A plot of luminosity against surface temperature or spectral type for a group of stars.
  3. 3. Middle-age stars that can be found running diagonally through the middle of an HR diagram.
  4. 5. An assemblage of stars, oval in shape, that contains no conspicuous interstellar material.
  5. 6. The outermost extent of a galaxy with a sparse distribution of stars.
  6. 7. A large assemblage of stars without radial symmetry.
  7. 9. A variable radio source of small angular size that emits very rapid radio pulses in very regular periods.
  8. 11. Two stars that revolve around each other.
  9. 12. One of the 107 galaxies, nebulas, star clusters, and other deep sky objects classified with an M followed by a number.
  10. 14. The main portion of a galaxy. Consists of a nucleus, bulge, and spiral arms.
  11. 19. A measure of the luminosity of an object like a star.
  12. 21. A star of large luminosity and radius.
  13. 28. The apparent displacement of a nearby star caused by the revolution of the Earth around the sun.
  14. 30. An object of very high redshift that looks like a star but is extragalactic and highly luminous.
  15. 31. The rate at which an object must travel in order to break free of the influence of gravity.