Which of the following)j2(b. bjvakomj6bi:uh210+bi he ku is correct for a stable star?

  1.A star X is burning carbonyistfoy s ,,++k*t xk; in its core. The reaction is given by:
$^{12}_{6}C$+$^{12}_{6}C$→$^{24}_{12}​Mg$
The following data are available for the reaction.
Rest mass of the$^{12}_{6}C$= 12.0111507u
Rest mass of the$^{24}_{12}​Mg$= 23.9909630u
Determine, in MeV, the energy released in the reaction. Be sure to express your answer to the correct number of significant figures. $ΔE$ =    MeV
2.The star Y is a red supergiant. State the next steps in the evolutionary sequence of the star Y.
3.Outline why the sun is not expected to undergo carbon fusion.

  Which of the following is correct about a red gianro 7z:1v 3wvvx9gsq t:t star?
I. The orbits of the inner planets of the solar system and could fit into the volume of it
II. Cooler than the Sun
III. Have higher luminosity than the Sun

  1.VV Cephei is a binary star system compose0 wk *ntto:gz(d of two stars referred to as VV Cephei A (t:z0 wg*oktn and VV Cephei B.
(1)The measured wavelength of the peak spectral line of VV Cephei A is 760 nm. Show that the surface temperature of VV Cephei A is approximately 3800 K. T =    K
(2)The surface temperature of the Sun is $T_⊙$​=5800 K. The luminosity of the VV Cephei A is $2.7\times10^5$ times the Sun's luminosity $L_⊙$​. Determine the radius of VV Cephei A in terms of the Sun's radius $R_⊙$​. R =    $R_⊙$​
3.A Herzsprung-Russel (HR) diagram is shown.


Plot the current position of VV Cephei A on the HR diagram and identify the classification of VV Cephei A.
2.The mass of VV Cephei B is about 11 times the mass of the Sun and it is not on the main sequence.
(1)In terms of forces, explain the condition that causes a star to first leave the main sequence.2
(2)Explain why VV Cephei B is likely to remain on the main sequence for a shorter time than the Sun.2
(3)The parallax angle for VV Cephei B is 0.31 arcseconds. Calculate, in light years, the distance between the earth and VV Cephei B.2. d =    ly
(4)State why the parallax method is not suitable for measuring the distance of very distant stars.

  A main sequence star has a mass greater than 4 times the mass t8/ c +eb1dmxroo l4o9of the Sun. Which of the following is correct about the possible the fate of the sxm+8bd4to r oe/l19o ctar?
I. White dwarf
II. Neutron star
III. Black hole

  A star with a mass of twvvl y iw;j(/e.ice the mass of the sun is a main sequence star. The time the sun is expected to spend in the main sequence is T. Which of the following is correct for the time the star is expwi(./ lv;v eyjected to spend in the main sequence and the next stage in its evolution?

  In the core of a star, a proton-proton chain b.:(vi cin*iylvi 5o8 reaction takes place.
$4^1_1​H$→$^4_2​He$+$2^0_{+1}​β^+$+$2\,ν_e$​+$2\,γ$
After the initial stage of the reaction, two positrons annihilate with electrons present in the surroundings. Which of the following correctly shows the nature of the chain reaction and the energy released due to annihilation?

  The parallax angles of Star A and Star B are 0.250 ab d1xdi0;fy 1wrcseconds and 0.500 arcseconds respectively. What is the shortest possible y;xbf1d 0i1 dwdistance, in parsec, between Star A and Star B?

  A star with a mass similar to the Sun, a temperature hotter than the Sun, 9m;ph5g xeo(iand a radius similar to the Earth would be found in which region of the usual Hertzsprung-Rus iegp 59(mhx;osell diagram?

  The luminosity of the Su9rwm rh7a1 ujyy(gy6156dzy xn is $L_⊙$​. A main sequence star with twice the radius of the sun and twice the temperature of the sun has a luminosity of $L$. What is the ratio of $\frac{L}{⊙​L}​$ ?

  Some regions on the H-R diagram are labelletvr9d 2 n c(+6hobd2rl3x1prud.

A main sequence star with a mass of three times the Sun will evolve through a series of stages. Which of the following sequences of stages could correctly represent the path of the evolution of this star?

  For fusion reactions to occur in a cloud of stellar dust,yd2uxk (ec82a4m2l yo 7ntjs, a combination of high temperature and high density among hydrogen nuclei is essentms,2kauo jy2 (xc 87n4ylted2 ial. Which of the following correctly shows why high temperature and high pressure are needed?