2. A body of matter Vague and Indistinct shape Dense mass No amount of light can break out Black Hole, Gravitational Force and Mass

3. Formed during a star’s death Examined and Observed by scientist Enormous quantity and volume Absolutely and completely black

4. Insufficient mass Cast of layers White dwarf Production of nuclear energy

5. Continued Orbit of the Planets Mass is needed, not sun There will be no changes If the Sun Becomes a Black Hole?

6. Star nameSolar mass (Sun = 1) R136a1 [1] 265–320 WR 101e150–160 HD 269810150 Peony Nebula Star150 LBV 1806-20130–200 HD 93129 A + B [2][3] A=120–127, B=80 HD 93250118 NGC 3603-A1A=116, B=89

7.  Infinite / Endless  It appears slower and slower through time  Very rapid

8.  About a quarter of the Universe  Black holes are ruled out  There will be no gamma rays

9.  There is gravitational force  Continued orbiting  Energy will be harness from intense mass

10.  Observed by scientists  Charted and Visually Represented