LEO ALHOTY SLES T ACTIVITY 6: MULTIPLE CHOICE
Directions: Choose the letter of the best answer. Write it on the spoce provided before the number
1. when trying to plan for your recreational activily, which should be the best thing to keep in minds
A. it should be your interest
B. will give you the chance to earn money
C. It should be away from home D. Within your comfort zone
2. Who is the founder of ZUMBA
A. Roberto Beto Reyes B. Roberi Beto Reyes
C. Roberto Berto Perez D. Robert Berto Perez
3. Activities during free time is called recreational activity. What is the primary reason why one engages in recreational
activity
A. Enjoyment B Fun
C. Fitness
D. Fundamentals
4. In hiking, what fitness component is required of you?
A. Speed
B. Agility C. Strength
D. Endurance
5. What is the most fundamental skill need in orienteering?
A. Setting the map B. Locating the points C. Running its speed D. Communicaling with groupmates
6. Why did William Morgan invent volleyball
A To make his client busy
B. To make fun out of nothing
C. To make his client physically fit D. To create an indoor activity during the winter season
7. Navigating an unfamiliar place requires a skill in?
A. Camping 8. Hiking C. Orienteering D. Mounteering
8. Why is badminton played indoors?
A. Its more convenient to play inside the gym B. Friction is greater providing better stability
C. Air resistance is lesser inside the gym
D. Its more comfortable inside the gym
9. In hiking, what should be the group's pacing?
A. The pace of the lead man
B The pace of the act man
C The pace of the slowest man
D the pace of the fastest man
10. In an outdoor activity, which of the following is not a natural frail sign?
A. Rocks
B. Grass
C. Twigs
D. Yarn​

  sequence  is a continuous and distinctive band of  stars  that appears on plots of stellar  color  versus  brightness. these color-magnitude plots are known as  hertzsprung–russell diagramsafter their co-developers,  ejnar hertzsprungand  henry norris russell. stars on this band are known as  main-sequence stars  or  dwarf stars. these are the most numerous true stars in the universe, and include the earth's  sun.after condensation and ignition of a star, it generates  thermal energy  in its dense core region through  nuclear fusion  of  hydrogen  into  helium. during this stage of the star's lifetime, it is located on the main sequence at a position determined primarily by its mass, but also based upon its chemical composition and age. the cores of main-sequence stars are in  hydrostatic equilibrium, where outward thermal pressure from the hot core is balanced by the inward pressure of  gravitational collapse  from the overlying layers. the strong dependence of the rate of energy generation on temperature and pressure to sustain this balance. energy generated at the core makes its way to the surface and is radiated away at the  photosphere. the energy is carried by either  radiation  or  convection, with the latter occurring in regions with steeper temperature gradients, higher opacity or both.the main sequence is sometimes divided into upper and lower parts, based on the dominant process that a star uses to generate energy. stars below about 1.5 times the  mass of the sun  (1.5  m☉) primarily fuse hydrogen atoms together in a series of stages to form helium, a sequence called the  proton–proton chain. above this mass, in the upper main sequence, the nuclear fusion process mainly uses atoms of  carbon,  nitrogen  and  oxygen  as intermediaries in the  cno cycle  that produces helium from hydrogen atoms. main-sequence stars with more than two solar masses undergo convection in their core regions, which acts to stir up the newly created helium and maintain the proportion of fuel needed for fusion to occur. below this mass, stars have cores that are entirely radiative with convective zones near the surface. with decreasing stellar mass, the proportion of the star forming a convective envelope steadily increases. main-sequence stars below 0.4  m☉undergo convection throughout their mass. when core convection does not occur, a helium-rich core develops surrounded by an outer layer of hydrogen.in general, the more massive a star is, the shorter its lifespan on the main sequence. after the hydrogen fuel at the core has been consumed, the star  evolves  away from the main sequence on the hr diagram, into a  supergiant,  red giant, or directly to a  white dwarf.