Which of the following is correct for a stable star?l2kcn/omr e(p+0-eazs- z a4qu2 xsh g4l, vv:

  1.A star X is burning carbon in itigf19lwy -f28 pidm3xs 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 following72 ,h .stdbtf(kwamw +.nq3qc is correct about a red giant 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 composed of two stars referred to as d/vno2q9m sr1rh3fm8 VV Cephei A 3s2fh9m d18n/qmorvrand 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 thew+ybdcq,p5t y 3or/8r mass of the Sun. Which of the following is correct about the possible the fate of thty53,q+c w/rp8d broy e star?
I. White dwarf
II. Neutron star
III. Black hole

  A star with a mass of twice the mass 2 l xro:.af2lsof the sun is a main sequence star. The time the sun is expected to spend in the main sequence is T. W.:xsor2llfa 2hich of the following is correct for the time the star is expected to spend in the main sequence and the next stage in its evolution?

  In the core of a star, a proton-proton chain reactioi q0 /ywgla7rp edt/04n 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 arcseconds and 0.500 a;xihn((v-w zn rcseconds respectively. What is (h;nv zwx(i-n the shortest possible distance, in parsec, between Star A and Star B?

  A star with a mass simil:fw ce :9jiq9dar to the Sun, a temperature hotter than the Sun, and a radius similar to the Earth would be found in which region of the usual Hertzsprung-Russell di9::wc jie9qdf agram?

  The luminosity of the Sue-.1qg2z2c d2 jzux- r(ij glgn 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 laptywh 9g9;g/s)tq m*vbelled.

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 ofnw q0bsj,pievrv c, 43y:1bh+ stellar dust, a combination of high temperature and high density among hydrogen nuclei is essential. Which of the fhci4bvbnrq s0y,,1 vj we p+3:ollowing correctly shows why high temperature and high pressure are needed?