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New Indivisible Planetary Science Paradigm J. Marvin Herndon
New Indivisible Planetary Science Paradigm J. Marvin Herndon

... Of the eight planets in the Solar System, the outer four (Jupiter, Saturn, Uranus, and Neptune) are gas-giants, whereas the inner four are rocky (Mercury, Venus, Earth, and Mars), without primary atmospheres. But the inner planets originated from giant gaseous protoplanets and their massive, primord ...
Are constellations just mythic figures in the sky?
Are constellations just mythic figures in the sky?

... Because of the Earth’s slightly oval (elliptical) orbit, its distance from the Sun changes throughout the year. We (in the northern hemisphere) are actually closer during our winter. ...
Foundation 1 - Discovering Astronomy
Foundation 1 - Discovering Astronomy

... Because of the Earth’s slightly oval (elliptical) orbit, its distance from the Sun changes throughout the year. We (in the northern hemisphere) are actually closer during our winter. ...
Physics Today - Earth, Environmental and Planetary Sciences
Physics Today - Earth, Environmental and Planetary Sciences

... The nature of our Moon The natural first step in understanding our Moon is to consider its composition. We’ve all heard the amusing myth that the Moon is made of green cheese, a theory that, astonishingly, has been tested (see box 1). The six Apollo Moon missions, conducted between 1969 and 1972, no ...
celestial clock - the sun, the moon, and the stars
celestial clock - the sun, the moon, and the stars

... day in the calendar because there are exactly 12 hours of daylight and 12 hours of night. On this day every place on Earth has almost exactly equal hours of night and day.4 The amount of time it takes for the earth to start at a spot where the Sun is directly above the Tropic of Capricorn and return ...
Dwarf Planets
Dwarf Planets

... Ice Ball ...
Introduction To Astronomy
Introduction To Astronomy

... • Stars and other things outside our solar system have a particular Right Ascension and Declination or RA and DEC (almost constant) • Earth’s Equator, North Pole, and South Pole line up with the Equator and North Pole, and South Pole, of the Celestial Sphere ...
The Night Sky This Month - Usk Astronomical Society
The Night Sky This Month - Usk Astronomical Society

... confused with the modern astrological phrase ‘supermoon’ devised in 1979 by an astrologer and whose arbitrary meaning is not as well defined. Astronomers should avoid the expression supermoon or its converse micromoon. This is a good time of year to observe a first quarter Moon. The Moon is still hi ...
The Celestial Sphere
The Celestial Sphere

... The diurnal path or the daily path of a star is a circle parallel to the celestial equator. Whether you can see a star or not depends on two things. First of all, the star must be above the horizon, and secondly it must be night. At any given place on the Earth, the celestial sphere consists of thr ...
Lecture 1: Properties of the Solar System Properties of the Solar
Lecture 1: Properties of the Solar System Properties of the Solar

... An average density is adopted for the Sun and it is assumed that the mass is mostly within 0.6R. This value is 0.72 for a perfect sphere, but the Sun is oblate. ...
Basic Observations of the Night Sky
Basic Observations of the Night Sky

... you can see in the illustration on the preceeding slide, this has the effect of making the Sun appear to rise higher in the sky and provides a longer period of daylight • In winter, we are tilted away – lower height to the Sun and shorter days ...
Chapter 10 - Macmillan Learning
Chapter 10 - Macmillan Learning

... 2. •Would the magnitude of the acceleration due to gravity near Earth’s surface increase more if Earth’s mass were doubled or if Earth’s radius were cut in half? Justify your answer. 3. •According to Equation 10-2, what happens to the force ­between two objects if (a) the mass of one object is doubl ...
evening star
evening star

... Venus, the jewel of the sky, was once know by ancient astronomers as the morning star and evening star. Early astronomers once thought Venus to be two separate bodies. Venus, which is named after the Roman goddess of love and beauty, is veiled by thick swirling cloud cover. ...
Johannes Kepler
Johannes Kepler

... orbit the sun and Copernican values for the periods of the planets. These values were sets of data points, each separated by 687 days which was known to be one Martian year. ...
Biological Adaptations - Hartsville Middle School
Biological Adaptations - Hartsville Middle School

... • Planets may have a terrestrial or rocky surface or a gaseous surface. Gaseous planets are considerably larger than terrestrial planets. • Planets may have rings. Some planets have a unique surface characteristic, for example color or an atmospheric storm. • Movement of planets is based on revoluti ...
Patterns in the Sky - Madison Public Schools
Patterns in the Sky - Madison Public Schools

... Earth orbits the Sun (revolves) once every year: • at an average distance of 1 AU ≈ 150 million kilometers. • with Earth’s axis tilted by 23.5º (pointing to Polaris) It rotates in the same direction it orbits, counterclockwise as viewed from above the North Pole. ...
Geology Lab Final Exam
Geology Lab Final Exam

... 1. Wind direction always moves from a. low pressure to high pressure b. high pressure to low pressure c. neutral pressure to high pressure d. compressional pressure to low pressure 2. The ozone layer is located in the a. stratosphere b. troposphere d. thermosphere ...
Earth Science Reference Tables Review
Earth Science Reference Tables Review

... 103. As a rocket passes through the mesopause, it enters which temperature zone of the atmosphere? 104. In which two temperature zones of Earth’s atmosphere does temperature increase as altitude increases? 105. Which visible wavelength of the electromagnetic spectrum has the shortest wavelength? 106 ...
RAW #17-February 14
RAW #17-February 14

... By Scientific American, adapted by Newsela staff ...
Scientific American`s Ask the Experts
Scientific American`s Ask the Experts

... steeply with decreasing size, but even at micrometer sizes the Pioneer spacecraft were hit only a few times during their passage. That is not to say that asteroids cannot pose any danger, however. It is worth noting that for a large planet like Earth, over a long period of time, there is an apprecia ...
Venus
Venus

... • Venus has highland areas that are as big as Australia. • There are more than 1,000 active volcanoes over 20 miles in size on Venus. • Venus’s surface is rocky. ...
Trainer`s Notes
Trainer`s Notes

... Sky Map. See: http://server1.sky-map.org/?locale=EN Stars 1 Honour Trainer’s Notes_Extra Info Edited by Dr B Hands, Queensland Wilderness Adventure Club. Also check out libraries of do a Google search on ‘Astronomy’. There’s heaps of information. ...
Jupiter
Jupiter

...  Jupiter is the biggest planet in the solar system.  Jupiter is 240 lbs in size.  The volume of Jupiter is 1.43128×1015 km³ . ...
1 Lecture 8: Uranus and Neptune
1 Lecture 8: Uranus and Neptune

... – pressure outside the core too low to form metallic hydrogen – origin of the magnetic field, like Uranus, is therefore probably very different than Jupiter and Saturn – possible “slushy” outer core with ammonia dissolved in water creating a thick electrically conducting layer – circulating currents ...
Seeing Through the Clouds of Venus
Seeing Through the Clouds of Venus

... •  The sun gets ~6% more luminous every 1 billion years •  As the sun gets brighter (hotter) with time, the region around the star where habitable planetary temperatures are possible gets pushed outward At  a  later  Sme:   Sun  is   brighter   ...
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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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