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4. Give reason a. Nothing is permanently at rest in the universe. b. All the gaseous masses in the universe do not change into stars, c. Black holes cannot be observed directly like other celestial bodies, d. The sun will not change into a black hole. e. Astronomical unit and lightyear are used as unit for measurement in astronomy.

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Feb 16,2025

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a. In the universe, everything moves due to gravitational forces and cosmic expansion, so nothing remains permanently at rest. b. Not all gaseous masses become stars because they may lack sufficient mass, density, or the right conditions needed for nuclear fusion. c. Black holes can't be seen directly because their gravity is so strong that not even light can escape, making them invisible to telescopes. d. The Sun won't turn into a black hole because it's not massive enough to collapse under its own gravity; instead, it will become a white dwarf after expanding into a red giant. e. Astronomical units and lightyears are used to measure distances in space, with 1 AU being the average distance from Earth to the Sun and 1 lightyear being the distance light travels in a year, making it easier to describe vast cosmic distances.

Solución

Below are the reasons for each statement: a. Nothing is permanently at rest in the universe.  Reason: In the universe, every object is influenced by gravitational forces from other objects and by the overall expansion of space. Even if an object appears to be at rest from one perspective, relative motion exists when viewed from another reference frame. In accordance with Newton's first law, an object remains in uniform motion unless acted upon by an external force; given the constant interactions (both gravitational and due to cosmic expansion), “absolute rest” is never achieved. b. All the gaseous masses in the universe do not change into stars.  Reason: For a gaseous mass to become a star, specific conditions must be met—such as sufficient mass (exceeding a critical threshold), appropriate density, and the ability to cool and collapse under gravity. Many gas clouds are too diffuse, fail to overcome internal pressure or turbulence, and may dissipate or form other structures (like planets or brown dwarfs) instead of igniting nuclear fusion to become stars. c. Black holes cannot be observed directly like other celestial bodies.  Reason: A black hole’s gravitational pull is so intense that not even light can escape from within its event horizon. This absence of emitted or reflected light means we cannot directly image black holes using conventional telescopes. Instead, their presence is inferred by observing the gravitational effects on nearby matter, radiation emitted from accretion disks, or the motion of stars near the black hole. d. The sun will not change into a black hole.  Reason: The formation of a black hole typically requires the collapse of a very massive star (usually several times the mass of the Sun) after it has exhausted its nuclear fuel, often after a supernova explosion. The Sun’s mass is insufficient to trigger this process. Instead, it will eventually expand into a red giant and ultimately shed its outer layers, leaving behind a white dwarf. e. Astronomical unit and lightyear are used as units for measurement in astronomy.  Reason: Distances in space are enormous compared to everyday scales, so it is practical to use units that simplify these measurements. An astronomical unit (AU), defined as the average distance between the Earth and the Sun, is useful for expressing distances within our solar system. A lightyear—the distance light travels in one year—is convenient for expressing vast interstellar or intergalactic distances. These units make it easier to communicate and comprehend the enormous scales found in the universe.

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The universe is in a constant state of motion due to the expansion of space itself, as described by the Big Bang theory. Even celestial bodies that may appear stationary are influenced by gravitational forces from nearby objects, causing them to orbit and move through the cosmos, ensuring that nothing remains truly at rest. While stars are formed from gaseous masses through processes like nuclear fusion, not all gas clouds have the right conditions or density to initiate star formation. Many factors, including temperature, turbulence, and interstellar pressure, play significant roles in determining whether a gas cloud will collapse and form a star, resulting in a diverse range of celestial outcomes beyond just stars.

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