Which one of the mechanism below can NOT be responsible for providing intrinsic luminosity for planets? Gravitational settling of the hydrogen molecules. Gravitational settling of the helium atoms. Residual heat dating from the formation epoch of the planets. Decay of radio-active isotopes like uranium.
Q: How do the planets in our solar system, for example Jupiter, affect the orbits of the other planets?…
A: The gravity of any particle in the Universe affects any other particle, no matter where these…
Q: Why do astronomers conclude that none of the Jovian planets' rings can be left over from the…
A: A ring or a ring system around a planet is made of dust and other solid materials. It is also called…
Q: a) Suppose the Earth grew to its present size in 1 million years through the accretion of particles…
A: Ques: Suppose the Earth grew to its present size in 1 million years through the accretion of…
Q: Which is these facts is NOT explained by the nebular theory? O There are two main types of planets:…
A: Number of planets pf each type (4 terrestrial and 4 jovian) This is not clearly explained by nebular…
Q: 12. Why is Jupiter so much riches in hydrogen and hellum than Earth?
A: Jupiter is the largest planet in our solar system and is located fifth from the Sun. It belongs…
Q: The cores of terrestrial planets are mostly metal because: O The entire planets are mostly metal…
A: option B is correct .( metals are denser and so sank to the centres of the planets when they were…
Q: What is the order of magnitude of "big G"? (Numerical answer).
A:
Q: 1) Why is life more likely to be found on the moons of the Gas Giants instead of on the Gas Giants…
A: (1) The main component of the gas giant is hydrogen and helium. But we know that life is made of…
Q: Why does the solar nebula theory predict that planetary systems are common?
A: The nebular hypothesis explains the planet's formation and evolution in our Solar System. It was…
Q: Using Wien’s displacement law, what is the peak wavelength of Earth if its surface temperature is…
A: The surface temperature of the Earth,
Q: Assume a reasonable density for a trans-Neptuian object with the same mass as Earth, located 50 AU…
A:
Q: What processes cleared the nebula away and ended planet building?
A: The four main reasons for clearing of protosolar nebula are : 1. Radiative Pressure : The light…
Q: Which of these views cannot be used when trying to detect exoplanets using the radial velocity…
A: Let's go through each of the three cases and explain why the views cannot be used for detecting…
Q: What appears to be the most common size of exoplanets? Jupiter size Neptune size…
A: Exoplanets are found outside of solar system. Their radii is 1.4 to 2.8 times the radius of earth.
Q: Compare and contrast the terrestrial planets to the gas giant planets. Be sure to include…
A: these are the comparison points of terrestrial planets to the gas giant planets (1) example of gas…
Q: The search for extrasolar planets fall broadly into two categories, what are they? Lensing and…
A: The search for extrasolar planets fall broadly into two categories, what are they.
Q: What is the range of density for the outer planets (in g/cm3)? 1.2 to 5.5 2.2 to 5.5 2.2 to 6.5 3.3…
A: Outer planets are less dense and having density about 1 g/cm3.
Q: 4b) the average density of the earth is 5.5 g/cm^3. Which has the greater density 1g of uranium of…
A: We are given with average density of earth i.e 5.5 grams per cubic cm
Q: L(1 – a) T = 4 40
A:
Q: An exoplanetary system has two known planets. Planet X orbits in 290 days and Planet Y orbits in 145…
A: Given data *The time period of the Planet X is Tx = 290 days *The time period of the Planet Y is Ty…
Q: While doing a transit study, you find an exoplanet around a nearby Sun-like star. The time between…
A: given, P= 32days t2−t1= 30minutes t3−t1= 5hours vr= 65m s−1 δF/F= 0.01 a. when the planet lies…
Q: What percentage of the mass of the solar nebula consisted of elements other than hydrogen and…
A:
Q: the
A: Due to the cold temperature in Neptune, the methane condenses in the higher layer of the atmosphere.…
Q: The Solar nebula was "mostly" b. hydrogen compounds: ammonia, methane and water c. heavier elements…
A: NEBULA:- A nebula is a giant cloud of dust and gas in space. Some nebulae come from yhe gas and dust…
Q: Jupiters moon, lo, loses about 870.0 kg/s of sulfur dioxide to Jupiters magnetosphere. Sulfur…
A: Given:- Jupiter's moon, lo, loses about 870.0 kg/s of sulfur dioxide to Jupiter's magnetosphere.…
Q: Planets in the habitable zone of their stars: O are so far from their stars that it is very…
A:
Q: To survive passage through without burning or breaking the ground, an asteroid mus A. at least 1,000…
A:
Q: Imagine that in the future, scientists plan on colonizing planets that orbit other stars. Based on…
A: SOlution:
Q: 1) How massive would Earth had been if it had accreted hydrogen compounds in addition to the sme…
A: It is required to calculate how massive would Earth had been if it had accreted hydrogen compounds…
Q: What produced the helium present in Jupiters atmosphere and inside Sun's core ?
A: When the universe was created in Big Bang the temperature was very high. Once the temperature cooled…


Step by step
Solved in 3 steps

- 1. Which of the outer planets have compositions dominated by the "ices" ingredient? Check the correct two. 2. Which of the outer planets have compositions dominated by the "gases" ingredient? Check the correct two. 3. Most of the spaceflight missions to the outer planets have been flyby missions, but two of them were orbiters. Which of these two spacecraft orbited giant planets? Check the correct two. (Hint: An orbiter might do a flyby of one planet and then go on to orbit a different planet.) 4. Jupiter's mass is how many times larger than the Earth's? Just type a number, no words or any other extra stuff. 5. Which of the outer planets has extreme seasons, with its rotational axis being tilted so much that it is practically in the plane of its orbit?Kepler-444 is one of many stars with terrestrial planets that is over 10 billion a) What do you think the spectral type of Kepler-444 might be? b) How do stars of this spectral type end their lives? c) If evolution followed a similar course on a habitable pranet around a star similar to Kepler-444, it would be 5 billion years more advanced than we are. Let’s try to project our future and see what happens. In particular, suppose our civilization gets motivated enough to colonize another planet. Kepler indicates that most stars have potentially habitable (and colonizable) planets, so roughly how far away is the typical “nearest" planet? d) The New Horizons probe on its way to Pluto took 9 years to travel 30 AU. If we could send colony ships with the same average speed, roughly how long would it take to reach the typical nearest planet? уears old.the co te on Pictor. The 270 TOI System TOI 270 c Earth 365-day orbit $1 AU from Sun Habitable 5.7-day orbit 0.05 AU $2.4 Earth radii Largest in system 59 F, 15 C 300 F, 150 C TOI 270 TOI 270 d M3-type dwarf star TOI 270 b $11.4-day orbit 0.07 AU 3.4-day orbit 2.1 Earth radii 0.03 AU Temperate 1.25 Earth radii Likely rocky 150 F. 67 C 490 F. 254 C Figure taken from https://exoplanets.nasa.gov/news/1593/tess-scores-hat-trick-with-3-new-worlds/ What makes the TOI-270 system particularly interesting is that the three exoplanets detected this far (there may be more) have sizes comparable to the Earth. Compare the orbital period of TOI 270 c and TOI 270 d. For every revolution that TOI 270 d makes around the host star TOI 270, how many revolutions does TOI 270 c make?
- 4) Science fiction movies often portray asteroid belts as crowded, dense regions that require spaceships to maneuver quickly to get through them. In this problem, we will calculate the fraction of volume in an asteroid belt that is actually occupied by asteroids. a) If there are 300,000 large asteroids between 2 and 3 AU from the Sun, and each asteroid is assumed to be spherical with a radius of 100 km, determine the total volume occupied by asteroids in this region. Recall that the volume of a sphere is given by the equation V = 4TR³ /3. b) Let's assume the region in which these asteroids orbit is an annulus with an inner radius of 2 AU, an outer radius of 3 AU, and a thickness of 2Ro. Determine the volume of this region. Recall that the area of a circle is given by the equation A = TR². Here are two conversions that you'll need: 1 AU = 1.496 × 108 km and 1 Ro = 6.955 × 105 km. c) What is the ratio of the volume occupied by asteroids to the volume of the asteroid belt (i.e., the…As a consequence of conservation of ............., the 2nd Law of Planetary Motion also implies that a planet will move ............ when farther away from its host star.Some astronomers argue that Jupiter and Saturn areunusual, while other astronomers argue that all solarsystems should contain one or two such giant planets.
- What is the frost line in the solar nebula? Explain how temperature differences led to the formation of two distinct types of planets.What is an exoplanet? Group of answer choices A planet in our solar system beyond Pluto. Any planet with extra-terrestrial life. A planet in an extra-solar star system outside of our solar system. Objects in the solar system such as Pluto that were once considered planets but no longer are.How would the solar system be different if the solar nebula had cooled, with a temperature half its actual value? [select all that apply] options: There would be more comets. Life would have been very unlikely to evolve here. There would be no comets. There would be fewer asteroids. There would be more asteroids. Jovian planets would have formed closer to Sun. Terrestrial planets would be large
- 2. The destructive "Tunguska Event" of 1908 seems to have been due to an airburst by a modest-sized asteroid a direct impact on land by a large asteroid an ocean impact by a comet a nearby supernova explosion Astronomers have determined that the probability of a significant asteroid impact on Earth during your lifetime is about the same as the probabilty that you'll win the lottery. True FalseThe microlensing technique for detecting extrasolar planets involves obtaining OBSERVING brightness measurements of a star and identifying brief, periodic dips in its brightness infrared images of a planet with the light from its host star blocked out a spectrum of a star and identifying periodic wavelength shifts in its features brightness measurements of a star and identifying a brief magnification in its brightness a spectrum of an extrasolar planet and identifying elements and compounds present in its atmosphereThe planet Uranus was discovered in 1781, and Neptune, the next planet outward from the Sun, was discovered in 1846. Imagine you're an astronomer in 1846, and you start wondering if there's another planet out beyond Neptune. You decide to try and discover its existence using the same method that was used for Neptune. How will you do this? Group of answer choices You'll recruit a large number of astronomers to use their telescopes to carefully scan the sky in directions that are far from the ecliptic. The regions around the north and south celestial poles will probably be the best "hunting grounds" for the new planet. You'll examine Uranus and Neptune very carefully, on every clear night, for several years, to see if you can find any evidence that sunlight has been reflected off of the `new' planet, then off of Uranus or Neptune, before arriving on Earth. On rare occasions when Neptune passes in front of the Sun, as seen from Earth, you'll look carefully at the Sun (with a safe…