Astronomy HOMEWORK Chapter 1 9th ed 5. In Figure 1-8, what is another name for the “Sun’s annual path?” Ecliptic. This term also refers to the mathematical plane of Earth’s orbit. 10. By about how many degrees does the Sun move along the ecliptic each day? The Sun moves 360 degrees in 365.25 days along the ecliptic, so Degrees per day = (360◦ )/365.25 days = 0.986◦ = 1◦ . Round to 1 degree since the question says “about how many...” 14. What are the vernal and autumnal equinoxes? What are the summer and winter solstices? How are these four events related to the ecliptic and the celestial equator? The equinoxes are the points on the celestial sphere where the ecliptic and celestial equator intersect. The vernal equinox is the point where the sun crosses the celestial equator northbound.…
It is easy to flip to the index of an astronomy textbook to discover that, say, the Sun lies 150 million kilometers away from Earth. It is far more difficult (if not impossible), however, to picture this distance in the human mind. In this exercise, we will learn to access the often unpalatable distances encountered in astronomy by simply scaling the huge distances to more recognizable, pedestrian numbers. So long as every distance within the system of interest is scaled by the same factor, we retain the meaningful information about relative distances between objects. This is exactly the same principle employed by map makers so that they can fit Texas, for example, onto a turnable page.…
Gliese 436b one component was initially thought to be hot "ice" in various exotic high-pressure forms which would remain solid even with the high temperatures, because of the planet's gravity. The planet could have formed further from its current position, as a gas giant, and migrated inwards with the other gas giants. As it arrived at the range, the star would have blown off the planet's hydrogen layer through a coronal mass ejection, a massive burst of gas and magnetic field arising from the solar corona released into the solar wind.…
A) All white-dwarf supernovae involve the explosion of stars of nearly the same mass. B) White-dwarf supernovae occur only among young and extremely bright stars. C) White-dwarf supernovae are common enough that we detect several every year. D) All white-dwarf supernovae have similar light curves, which makes them easy to distinguish from massive-star supernovae. E) White-dwarf supernovae are so bright that they can be detected even in very distant galaxies. 50) What do we mean by the singularity of a black hole? A) It is the center of the black hole, a place of infinite density where the known laws of physics cannot describe the conditions. B) An object can become a black hole only once, and a black hole cannot evolve into anything else. C) There are no binary black holeseach one is isolated. D) It is the "point of no return" of the black hole; anything closer than this point will not be able to escape the gravitational force of the black hole. E) It is the edge of the black hole, where one could leave the observable universe. 51) Which of the following is an example in which you are traveling at constant speed but not at constant velocity? A) driving around in a circle at exactly 100 km/hr B) rolling freely down a hill in a cart, traveling in a straight line C) jumping up and down, with a period of exactly 60 hops per minute D) driving backward at…
2. A G2 I star is larger in diameter and more luminous than the sun.…
The massive star is a stage before the red supergiant.The way a massive star is formed is by fusing material into more heavier elements.The…
The area on the H-R diagram where “normal” stars can be found is known as the _________.…
4. Describe the difference in stellar evolution of stars the size of our sun with that of stars 4+ times larger than our sun. Include all of the steps and the causes of each step.…
The stars are the majority and most widely acknowledged astronomical components that symbolize the most essential development of the galaxies. The disbursement, age, and the framework of the night sky in the galaxy maintain a record of the heritage, evolution and characteristics of our galaxy. More important the stars are integral to the fabrication and allocation of heavy elements. Notably corresponding to oxygen, carbon, and nitrogen, is intimately associated with the capabilities of the planetary models, which in turn associate about them. Previously, the analysis of the conception, longevity, and…
Q1) Last night you saw the star Betelgeuse exactly on your eastern horizon at 5:47 PM. Two students are discussing their answer to the question "At 5:47 PM tonight where will you see Betelgeuse?"…
This region becomes known as the First Hydrostatic Core. The collapse is now essentially stopped. The core continues to rise in temperature, according to the virial theorem. The core is further heated by gas falling towards this region that create shockwaves, the core can reach temperatures of temperatures of 2000 – 3000 K. Once the density reaches approximately 10−8 g / cm3, of the material that is infalling, the star has reached a level of transparency that allows energy to be radiated from it. The radiation of energy away from the star’s exterior combined with the convection of energy in the star’s interior allow for it to contract further. The star will continue to contract until the gas within the star is hot enough to create internal pressure inside the star that can support the star’s structure from anymore gravitational collapse. When this happens the stars can be said to be in a state called hydrostatic equilibrium. A star in hydrostatic equilibrium has reached temperatures high enough for nuclear fusion of hydrogen to happen. For a more-massive protostar, the core temperature will reach 10 million kelvin at some stage, initiating the proton–proton chain reaction and allowing hydrogen to fuse, first to deuterium and then to helium. In stars of slightly over 1 M☉, the carbon–nitrogen–oxygen fusion…
The third thing that fascinates scientists’ minds is how did the galaxies form? The first theory states that the galaxies collapse as single objects out of gas clouds. More and more gas falls in the galaxy because of the gravity and it starts spinning. The other theory is that galaxies of gas gravitate together and form a new galaxy. During a long time, a lot of galaxies are formed together like this. Despite the fact that we really don’t know what exactly happened, some kind of merging took place. The main question is that do gas-galaxies that merged together, had stars in them or they came into being within the galaxy. The third theory is that black holes brought the galaxies together because they are in the centre of almost all the galaxies. The stars evolving around the black hole were the lucky ones that weren’t sucked in by the black hole.…
The planet Mercury is the closest to the sun. Mercury is the smallest planet in the solar system. This planet has an iron core in the center that makes it look wrinkly. The next planet that comes after Mercury is Venus. The planet was named after the Roman goddess Venus, who was the goddess of love. Venus is also called the morning and evening star, because of how bright it shines. It is in the like manner as earth, the only difference they have is Venus contains no life on its planet. ("Solar System Facts: Interesting Facts about Our Solar System." The Planets. N.p., 2010-2016. Web. 09 May 2016. ) Earth is the only planet not named after a Roman god. Additionally earth contains the only life existence on the planet. There is only one moon…
We begin by identifying two types of families of planets, rocky terrestrials and gaseous jovians. The latter planet made of gas with no solid surface. The atmospheres of these gaseous giants show a thicker density as you move closer to the core. However, unlike Earth’s rocky surface a gaseous jovian cannot be stood on. The four gaseous jovians in our solar system are Jupiter, Saturn, Neptune, and Uranus. Rocky terrestrials are the types of planets that possess a solid surface made of rock. Mars, Venus, and Mercury are examples of rocky terrestrials in our solar system. Of course, Earth is one of them as well.…
Bibliography: Works Cited Field, J. V. (1995 August). Home page. [Online]. [2000, Feb. 8]. Astronomy 161 "The Solar System" . [Online]. University of Florida. [2000, Feb. 8]. Landry, Peter (1999 June). Home page. [Online]. Dartmouth, Nova Scotia. CANADA. [2000, Feb. 8].…