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4.1 The Concepts of Force and Mass
4.1 The Concepts of Force and Mass

... • 3rd Law (of force pairs)  every satellite must also pull back. That is gravitational pulls on both bodies. • All the satellites must also be pulling each other (Earth and Mars). Why the gravity be restricted to astronomical bodies. It should also be between smaller bodies? ...
slooh celebrates dwarf planet night with ceres dancing with asteroid
slooh celebrates dwarf planet night with ceres dancing with asteroid

... same small piece of sky while also being easily visible through backyard telescopes. Both are unique.  Vesta is the only asteroid that sometimes reaches naked­eye visibility, thanks to being whiter than any  other. Ceres is spherical, possibly contains a thin atmosphere like Pluto, and, also like Pl ...
HOLIDAYS HOME WORK
HOLIDAYS HOME WORK

... Q7. The coefficient of viscosity (n) of a gas depends on the mass 'm' , the effective diameter 'd' and mean speed ' of the gas molecules. Use dimensional analysis to find n . METHODS OF MEASUREMENT Q1. What is the value of one i) 1o ii) 1' and iii) 1" in radian? Q2. Angular diameter of sun, as obser ...
Chapter 3: Galileo, Newton, and Einstein
Chapter 3: Galileo, Newton, and Einstein

... shape every point of which is the same total distance from two fixed points (the foci). Eccentricity is the distance between the foci and its center divided by half the longest distance across (semi-major axis). ...
Collisions with Comets and Asteroids
Collisions with Comets and Asteroids

... out of its original orbit into an increasingly eccentric one. The asteroid may either leave the solar system or move in toward the terrestrial, rocky planets. Eventually, such vagrants collide with Mars, the earthmoon system, Venus, Mercury or even the sun. A major fragment enters the inner solar sy ...
Earth and beyond
Earth and beyond

... A solar eclipse when the Moon only covers part of the Sun. The different shapes the Moon seems to have at ...
Solar System`s Age - Empyrean Quest Publishers
Solar System`s Age - Empyrean Quest Publishers

... Bang, which created the universe 13.7 billion years ago. • All heavier elements were manufactured by stars later. – Thermal-nuclear fusion reaction in the interior of stars – Violent explosions, so called supernovae that make the end of massive stars • As stars die, they eject material containing he ...
Celestial Objects
Celestial Objects

... Precession 6 – The Earth behaves somewhat like a spinning top, causing the axis of rotation to trace out a circle. This slow conical motion of the Earth’s axis of rotation is called precession, and is due to the gravitational effects of the Sun and Moon on the Earth’s equatorial bulge. Precession sl ...
1 light year = 9 x 10 12 km
1 light year = 9 x 10 12 km

... • The farther we look out in the Universe, the farther back in time we see. ...
The Earth in Space and finding where we are.
The Earth in Space and finding where we are.

... In 1727 John Harrison started building clocks to attack the problem of longitude…. Isaac Newton (who was on the search committee was convinced that no clock would ever be invented that could do the job…) John Harrison developed a highly accurate clock which proved to lose only 1.25 minutes in a 2 mo ...
Diameter of the Milky Way
Diameter of the Milky Way

... today is approximately equal to the number of grains of sand on all the beaches of Earth!! ...
Ans. - Testlabz.com
Ans. - Testlabz.com

... Ans. A football which is placed near us will appear more bigger than a football placed at a distance of 100 m. Q.33. The star Alpha Centauri is at a distance of about 40,000, 000,000,000 km from the Earth. Can you read this distance in kilometers conveniently? Ans. 40,000,000,000,000 = 4 × 1013 km. ...
Our Sun Produces Bizarre Radiation Bursts—Now NASA Knows Why
Our Sun Produces Bizarre Radiation Bursts—Now NASA Knows Why

... Closer to home, solar flares can also produce gamma rays. Flares happen when active regions on the sun suddenly release explosions of magnetic energy. That accelerates particles to incredibly high speeds and creates intense bursts of light that can briefly outshine the sun itself. (Also see “How Su ...
PLANETARY MOTION
PLANETARY MOTION

... ). The button play brings back the flow of time to its standard rate. In order to see the planet revolution, select each planet to see its orbit, zoom in or out from the Sun to see all the Solar System or only the internal planets. Observe that planets more distant from the Sun have a longer revolut ...
Section 3: Three Periodicities - Wobble, Tilt, and
Section 3: Three Periodicities - Wobble, Tilt, and

... because of the rotation of the Earth on its axis (that same rotation that gives us day and night), the other stars seem to be circling a stationary North Star. They're not, of course - but the rotation of the Earth makes it look as if they are. ...
PLANETARY MOTION G. Iafrate(a) and M. Ramella(a) (a) INAF
PLANETARY MOTION G. Iafrate(a) and M. Ramella(a) (a) INAF

... ). The button play brings back the flow of time to its standard rate. In order to see the planet revolution, select each planet to see its orbit, zoom in or out from the Sun to see all the Solar System or only the internal planets. Observe that planets more distant from the Sun have a longer revolut ...
Direct Detection of Exoplanets
Direct Detection of Exoplanets

... Even if we can image an Earth-like planet in the habitable zone of some star, we will not be able to resolve its surface features in the foreseeable future. (No “zooming in” to see oceans, forests, city lights… Later we’ll see how you can detect some of these through reflected light.) Instead, we mu ...
SNAKE RIVER SKIES Pomerelle Mountain Star Party
SNAKE RIVER SKIES Pomerelle Mountain Star Party

... Jupiter is the big story this month. It will be at its biggest and brightest at midmonth. This month will be the prime time to observe it. The dependable Perseid Meteor Shower peaks August 11th and 12th but the Moon will interfere. Mercury will sit very low in the sunset twilight in the west. It sho ...
Name
Name

... the sunset position will shift from northwest (first day of summer) to west (first day of autumn) to southwest (first day of winter) and back to west (first day of spring). This constant shifting is caused by the fact that Earth’s axis is “tilted” by 23.5 degrees. As a result, the ecliptic does not ...
What Makes a Planet Habitable?
What Makes a Planet Habitable?

... The youngest stages of planets Planets form and grow in so-called protoplanetary disks, which are huge gas and dust disks orbiting the youngest stars at ages of only one to a few million years, with sizes larger than the entire solar system. Dust particles coagulate in disks to ever larger grains an ...
Objects in the Sky STair
Objects in the Sky STair

... light it is reflecting from the sun which makes the different phases. ...
Chapter 13 Exploring the final frontier
Chapter 13 Exploring the final frontier

... 27. Use Kepler’s law of periods to determine the time required for the following planets to complete an orbit of the Sun. The radius of the Earth’s orbit is 150 × 106 km. 28. Jake the flying ace needs to hide his new experimental high-velocity plane in the hangar, away from the view of foreign spy s ...
Lab #5 (Feb 27
Lab #5 (Feb 27

... rotation period, relative to a distant, non-moving reference frame (the stars). The solar day is the time it takes for the Moon to complete a cycle of phases as seen from Earth.! ...
Gravitation and Orbital Motion
Gravitation and Orbital Motion

... times larger than the Earth’s radius, RE. What is the gravitational field strength at the surface of this newly discovered planet? Gravitational field strength of the new planet, gN, is Fg/m where the 2 interacting masses are the mass of the new planet, MN and m. At the surface, the distance between ...
PH2213 : Examples from Chapter 6 : Gravitation Key Concepts Two
PH2213 : Examples from Chapter 6 : Gravitation Key Concepts Two

... That’s a generic result for any small body orbiting around a larger (much heavier) one that can be treated as not moving. It shows that T 2 is proportional to r3 , as noticed hundreds of years ago for the planets orbiting the sun, and for moons orbiting Jupiter. The constant of proportionality depen ...
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Comparative planetary science

Comparative planetary science or comparative planetology is a branch of space science and planetary science in which different natural processes and systems are studied by their effects and phenomena on and between multiple bodies. The planetary processes in question include geology, hydrology, atmospheric physics, and interactions such as impact cratering, space weathering, and magnetospheric physics in the solar wind, and possibly biology, via astrobiology.Comparison of multiple bodies assists the researcher, if for no other reason than the Earth is far more accessible than any other body. Those distant bodies may then be evaluated in the context of processes already characterized on Earth. Conversely, other bodies (including extrasolar ones) may provide additional examples, edge cases, and counterexamples to earthbound processes; without a greater context, studying these phenomena in relation to Earth alone may result in low sample sizes and observational biases.
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