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Here - ScienceA2Z.com
Here - ScienceA2Z.com

... A planet is any object in orbit around the Sun that has enough mass to form itself into a spherical shape and has cleared its immediate neighborhood of all smaller objects. By this definition, the Solar System has eight known planets: Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, and Neptun ...
Motion of the Moon Phases of the Moon
Motion of the Moon Phases of the Moon

... • Lunar eclipses do not occur every month because the Moon’s orbital plane is tilted by 5 degrees with respect to the ecliptic – a total lunar eclipse occurs when the Moon crosses the ecliptic at full Moon – since the Earth’s shadow is much bigger than the Moon, total lunar eclipses occur more often ...
Feb 2017 - What`s Out Tonight?
Feb 2017 - What`s Out Tonight?

... The planets are best observed with a telescope using magnifithat were born out of the same nebula cloud. A group often forms cations from 50x to 200x. The five naked-eye planets are Mera pretty pattern. The Pleiades and Praesepe are great examples. cury, Venus, Mars, Jupiter and Saturn. Venus is ext ...
Other Bodies in the Solar System
Other Bodies in the Solar System

... • In 1801 Giuseppe Piazzi discovered the planet “Ceres” • William Herschel categorized Ceres and the other dwarf planets as asteroids , “star like” http://upload.wikimedia. org/wikipedia/commons/ 9/92/Giuseppe_Piazzi.jpg ...
paper
paper

Detecting the glint of starlight on the oceans of distant planets
Detecting the glint of starlight on the oceans of distant planets

... will appear darker than a Lambertian disk near full illumination. Finally, we show that planets with a mixed land/water surface will polarize the reflected signal by as much as 30–70%. These results suggest several new ways of directly identifying water on distant planets. © 2008 Elsevier Inc. All r ...
TRAPPIST: TRAnsiting Planets and PlanetesImals Small Telescope
TRAPPIST: TRAnsiting Planets and PlanetesImals Small Telescope

... The hundreds of exoplanets known today allow us to place our own Solar System in the broad context of our own Galaxy. In particular, the subset of known exo­ planets that transit their parent stars are key objects for our understanding of the formation, evolution and properties of planetary systems. ...
Jovian Planets Notes
Jovian Planets Notes

... 1) The rings extend far out in Saturn’s equatorial plane, and are inclined to the planet’s orbit 2) Over a 30 year period, we sometimes see them from above their northern side, sometimes from below their southern side, and at intermediate angles in-between a) When seen edge-on, they are almost invis ...
Neptune - Midland ISD
Neptune - Midland ISD

...  A new possible moon was discovered in 2013 orbiting 65, 400 miles away from Neptune.  It is expected to be no more than 12 miles across, making it the smallest ...
Cosmic Samples & Origin of Solar System
Cosmic Samples & Origin of Solar System

... from their interior and the impacts of volatilerich debris from the outer solar system It is likely that all the terrestrial planets originally had similar atmospheres Mercury and the Moon were apparently too small to retain their atmospheres Venus seemed to have experienced a runaway greenhouse eff ...
Solar System Formation
Solar System Formation

... circumstellar debris disk first imaged by Smith & Terrile (1984) disk almost edge on, extends beyond 2000 AU (!) at optical wavelengths temperature/color profile indicates large blackbodies not present ...
Lecture 6
Lecture 6

... 10 © 2004 Pearson Education Inc., publishing as Addison-Wesley ...
Stratigraphy and composition of lava flows in Mare Nubium
Stratigraphy and composition of lava flows in Mare Nubium

... leftover debris from the planet building process – things like comets and asteroids. With its powerful gravity, Jupiter sucked up many of them and also kicked lots of them out of the Solar System that could have hit Earth. Because of this, Jupiter is sometimes called the Solar System’s vacuum cleane ...
Mercury_Orbit_Lab_1_(better_than_2)
Mercury_Orbit_Lab_1_(better_than_2)

UNIVERSAL GRAVITATION
UNIVERSAL GRAVITATION

... Deviations in the orbit of Uranus led two astronomers to predict the position of another unobserved planet. This is how Neptune was added to the Solar System in 1846. Deviations in the orbits of Uranus and Neptune led to the discovery of Pluto in 1930 Most discoveries of new things are made by accid ...
What is a planet? - X-ray and Observational Astronomy Group
What is a planet? - X-ray and Observational Astronomy Group

... • There are two main models which have been proposed to • describe the formation of the extra-solar planets: – (I) Planets form from dust which agglomerates into cores which then accrete gas from a disc. – (II) A gravitational instability in a protostellar disc creates a number of giant planets. ...
PDF Version
PDF Version

... brightness that we can see ourselves, is equal to the intrinsic brightness divided by the square of the distance from us to the star. Astronomers used Cepheid variables in a nearby galaxy, which are all about the same distance from us, to find the correlation between the period and the intrinsic bri ...
Formation of the Solar System
Formation of the Solar System

... changes in the sky form this star – the astrometric technique, but this is difficult. • Since 1995, this Doppler Technique has found evidence of over 200 planets orbiting stars in the near vicinity of the Sun. • Some of the extrasolar planets can be detected when the transit the star. The star’s bri ...
Lab 3: The Galilean Revolution
Lab 3: The Galilean Revolution

... Next you are going to measure the orbit of one of your planet's moons: If your planet is Jupiter, you will measure the orbit of Ganymede. If your planet is Saturn, you will measure the orbit of Titan. If your planet is Uranus, you will measure the orbit of Oberon. If your planet is Neptune, you will ...
Formation and Detectability of Terrestrial Planets around
Formation and Detectability of Terrestrial Planets around

... components to constrain the binary orbital parameters. (See their reference list for an historical listing of publications relating to observations of α Cen A and B.) A similar study had been done by Pourbaix et al. (1999). In the earlier study, after fitting for the binary orbit, they examined the ...
First Exam - University of Iowa Astrophysics
First Exam - University of Iowa Astrophysics

... (d) an imaginary point on the celestial sphere which we see as straight overhead (e) an imaginary line of the sky, defined by the right ascension = 0 hours 18. Which of the following planets is most similar to the Earth in mass and diameter? (a) Venus ∗ (b) Jupiter (c) Saturn (d) Uranus (e) Mercury ...
Inquiry Plan, Year 5/6 - Owairoa Primary School
Inquiry Plan, Year 5/6 - Owairoa Primary School

... centre of our solar system and that it has eight planets: Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus and Neptune (Pluto as a ‘dwarf planet’). They should understand that a moon is a celestial body that orbits a planet (Earth has one moon; Jupiter has four large moons and numerous smaller o ...
What is the sun?
What is the sun?

... the sun in an orbit towards the sun, it is summer on that part of the Earth , Half a year later, the Earth goes round to the other side of its orbit. That part of the earth is now farther away from the sun and has it winter and the other part has its summer, Between wummer and winter, both halves of ...
Apr 2016 - Bays Mountain Park
Apr 2016 - Bays Mountain Park

THE LIFE CYCLE OF A STAR
THE LIFE CYCLE OF A STAR

... A star is a luminous globe of gas producing its own heat and light by nuclear reactions (nuclear fusion). They are born from nebulae and consist mostly of hydrogen and helium gas. Surface temperatures range from 2000C to above 30,000C, and the corresponding colors from red to blue-white. The brighte ...
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Definition of planet



The definition of planet, since the word was coined by the ancient Greeks, has included within its scope a wide range of celestial bodies. Greek astronomers employed the term asteres planetai (ἀστέρες πλανῆται), ""wandering stars"", for star-like objects which apparently moved over the sky. Over the millennia, the term has included a variety of different objects, from the Sun and the Moon to satellites and asteroids.By the end of the 19th century the word planet, though it had yet to be defined, had become a working term applied only to a small set of objects in the Solar System. After 1992, however, astronomers began to discover many additional objects beyond the orbit of Neptune, as well as hundreds of objects orbiting other stars. These discoveries not only increased the number of potential planets, but also expanded their variety and peculiarity. Some were nearly large enough to be stars, while others were smaller than Earth's moon. These discoveries challenged long-perceived notions of what a planet could be.The issue of a clear definition for planet came to a head in 2005 with the discovery of the trans-Neptunian object Eris, a body more massive than the smallest then-accepted planet, Pluto. In its 2006 response, the International Astronomical Union (IAU), recognised by astronomers as the world body responsible for resolving issues of nomenclature, released its decision on the matter. This definition, which applies only to the Solar System, states that a planet is a body that orbits the Sun, is massive enough for its own gravity to make it round, and has ""cleared its neighbourhood"" of smaller objects around its orbit. Under this new definition, Pluto and the other trans-Neptunian objects do not qualify as planets. The IAU's decision has not resolved all controversies, and while many scientists have accepted the definition, some in the astronomical community have rejected it outright.
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