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script (powerpoint)
script (powerpoint)

... symbol denotes the first 2009 epoch. The upper-right small panel shows a zoomed version of e's astrometry including the expected motion (curved line) if it is an unrelated background object. Planet e is confirmed as bound to HR 8799 and it is moving 46 ± 10 mas/year counter-clockwise. The orbits of ...
an Educator`s GuidE
an Educator`s GuidE

... These exoplanets are very far away, so how do we actually “see” them? Exoplanets are nearly impossible to photograph in the traditional sense, so we have to find them by observing the effects they have on their parent stars. These effects, driven by gravity and line-of-sight, are visible to us as ei ...
Lecture7_2014_v2
Lecture7_2014_v2

... Many bodies in Solar System just look like they’ve been hit! ...
The Cosmic Cupboard
The Cosmic Cupboard

Disk Instability Models
Disk Instability Models

... • Surface T = 50 K means lower midplane T • No artificial viscosity so no irreversible heating in shock fronts and a =0 assumed • Cooling time ~ 1-2 P ...
Comets - Astronomy @ Walton High School
Comets - Astronomy @ Walton High School

... metal, they can also contain organic compounds. Asteroids are similar to comets but do not have a visible coma (fuzzy outline and tail) like comets do. Meteoroid •A meteoroid is a small rock or particle of debris in our solar system. They range in size from dust to around 10 metres in diameter (larg ...
Can we detect asteroid impacts with rocky extrasolar planets?
Can we detect asteroid impacts with rocky extrasolar planets?

... or ratio of the fireball luminosity to the Sun’s luminosity, is proportional to the square of the diameter ratio and the fourth power of the temperature ratio: Relative luminosity = (Fireball diameter/Sun diameter)2 x (Fireball temperature/Sun temperature)4 The Chicxulub fireball works out as having ...
PDF only - at www.arxiv.org.
PDF only - at www.arxiv.org.

... Asteroids (NEAs) ke Jovian-crosser asteroid. Kata kunci: Asteroid, Element orbit, Tata surya, Masalah N-benda Jovian-crosser asteroids. The groups of NEAs are presented in Table 1. Investigation of orbital evolution of 3552 Don Quixote had already been done by taking into account all the planets in ...
Sample pages 1 PDF
Sample pages 1 PDF

... minutes, and/or seconds, as seen from Earth. OK, let’s define the three words in that sentence. A degree is 1/360 of a circle. Said another way, a circle contains 360°. A minute (short for minute of arc or arcminute) is 1/60 of 1°. A second (short for second of arc or arcsecond) is 1/60 of 1 minute ...
Origin of the orbital architecture of the giant planets of the Solar
Origin of the orbital architecture of the giant planets of the Solar

... The final semimajor axes of the planets are an important diagnostic of migration models. The simulations of compact systems in ref. 11 always produced final configurations in which Neptune was at ,30 AU, but Uranus was too close to the Sun. Our model nicely solves this nagging problem. As shown in F ...
Solar system and eclipse
Solar system and eclipse

... 5. There's a recurring myth that pregnant women can't go outside during an eclipse. Astronomers from the Griffith Observatory in LA say they get dozens of calls about it when an eclipse happens, even though it seems irrational. But if one of your friends is pregnant, don't worry, you can invite them ...
The outer solar system:
The outer solar system:

Primary and secondary eclipse spectroscopy with JWST: exploring
Primary and secondary eclipse spectroscopy with JWST: exploring

... chemistry composition instead of kinetics and photochemistry, simple cloud models, decoupling of radiative, dynamical and chemical processes) and would suffer from the incompleteness of the required physical/chemical data (spectroscopic data, kinetic rates). For low-mass rocky and icy planets, the si ...
asteroid
asteroid

... Asteroids, Comets, and Meteoroids Asteroids are small, rocky objects. The name “asteroid” actually means ‘star-like bodies’. ...
The Earth in space: An essay on the origin of the Solar system
The Earth in space: An essay on the origin of the Solar system

... me the Sun and a passing star were supposed to collide. In order to account for almost circular orbits of the planets, it was postulated that at that time the Sun was surrounded by a uniformly rotating gaseous envelope, which helped to turn the originally elongated planetary orbits into regular circ ...
Trimester 1 Exam –Science 6 S C I E N C E    6 TRIMESTER I EXAM
Trimester 1 Exam –Science 6 S C I E N C E 6 TRIMESTER I EXAM

... B This model places the Sun at the center of the Solar System with all planets orbiting the Earth. C This theory suggests the Universe was created with a single cosmic explosion. The Universe continues to expand at an increasing rate as a result of this explosion. Which of the above describes the ge ...
Jupiter - V
Jupiter - V

... Something REALLY Cool!!! • I am 11 years old on Earth ...
Extra-Solar Life: Habitable Zones
Extra-Solar Life: Habitable Zones

... • The ingredients of (Earth-like) life are all common: • H2O • C • Fe • etc. • So are many possible alternatives to them (i.e. Si, NH3, etc.) • Why are these so common? • If they are so common, why isn’t there life on ALL the planets? ...
PPT
PPT

... Many bodies in Solar System just look like they’ve been hit! ...
Looking for life in unlikely places: reasons why planets may not be
Looking for life in unlikely places: reasons why planets may not be

... intensity of light. For those of you who are not amateur astronomers, here are the magnitudes of the planets in the outer part of the solar system : Jupiter minus 2, Saturn plus 1, Uranus 6, Neptune 8, Pluto 15. Adding one to the magnitude means making the light fainter by a factor of 2.5. Now suppo ...
Eccentricity
Eccentricity

... Eccentricity and Elliptical Orbits All planets revolve around the Sun in an elliptical orbit. The name of that shape is an ellipse. An ellipse is an oval shape. ...
Measuring the ligth
Measuring the ligth

... Where f is the flux at the earth and fo a constant. To be noted in this formulae is the logarithm (The Hipparcos eye had a more or less logarithmic response, like any human), the minus sign (accounting for the fact that the more brilliant stars have the lower magnitudes like in the Hipparcos categor ...
YSO/PMS disk types, time-scales and evolution from 1
YSO/PMS disk types, time-scales and evolution from 1

... The initial sample had photometry for 1024 YSO candidates with estimated ages of 1 -10 Myrs Encompassing the timescales of disk dissipation previously observed for low mass stars and probing slightly different environments ...
Uranus and Neptune Uranus Saturn Neptune
Uranus and Neptune Uranus Saturn Neptune

... The Kuiper Belt consists _______. A.very soft leather used by Gerard Kuiper to make designer belts. B.asteroids that pass closer to the Sun than Earth's orbital distance. C.a region in the asteroid belt where all the Kuiper family objects orbit the Sun. D.mostly of small, icy planetesimals that for ...
Neptune
Neptune

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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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