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... –  Transit missions will be capable of finding Earth-like planets that cross in front of their stars. –  Astrometric missions will be capable of measuring the "wobble" of a star caused by an orbiting Earth-like planet. –  Missions for direct detection of an Earth-like planet will need to use special ...
Transiting exoplanets from the CoRoT space mission
Transiting exoplanets from the CoRoT space mission

... comparing observations during predicted transit-times with observations out of transit. Time-series follow-up is described in more detail in Deeg et al. (2009). Figure 3 shows that the field is rather crowded around the target star (labeled with a T). For any nearby star around the Corot-23 target, ...
Chapter 13 Power Point Lecture
Chapter 13 Power Point Lecture

... • A Sun-like star is about a billion times brighter than the light reflected from its planets. • Planets are close to their stars, relative to the distance from us to the star. – This is like being in San Francisco and trying to see a pinhead 15 meters from a grapefruit in Washington, D.C. ...
The Cosmic Perspective Other Planetary Systems: The New Science
The Cosmic Perspective Other Planetary Systems: The New Science

... •  GAIA is a European mission planned for 2013 that will use interferometry to measure precise motions of a billion stars © 2014 Pearson Education, Inc. ...
Opportunity Approaching Mountain Climbing Goal and Signs of
Opportunity Approaching Mountain Climbing Goal and Signs of

... Watching the fireworks tonight? As you're waiting for them to begin, point out to people some sky sights. The two brightest stars of summer, Vega and Arcturus, are high overhead toward the east and southwest, respectively. Far below Arcturus are the planet Saturn and, to its lower right, Spica. Near ...
Chapter 13 Other Planetary Systems: The New Science of Distant
Chapter 13 Other Planetary Systems: The New Science of Distant

... Learn That Other Stars Are Suns? • Ancient observers didn’t think stars were like the Sun because Sun is so much brighter. • Christian Huygens (1629–1695) used holes drilled in a brass plate to estimate the angular sizes of stars. • His results showed that, if stars were like Sun, they must be at gr ...
The Mt John University Observatory search for Earth
The Mt John University Observatory search for Earth

... solar neighbourhood with high temporal cadence. Owing to the extreme observational effort, these searches have to be dedicated to a few systems rather than to include as many targets as possible. The need of RV searches to focus on nearby bright stars has an attractive side-effect: the targets are a ...
The Search for Exoplanets - Worcester Polytechnic Institute
The Search for Exoplanets - Worcester Polytechnic Institute

... being large gas giants like Jupiter or Saturn, while others are small and rocky, like Earth and Mars. Exoplanets are almost always found to be gravitationally bound to a stellar system, however, there is at least some evidence to suggest that there may be a small minority of “rogue exoplanets” that ...
13_Lecture_Outline
13_Lecture_Outline

... Learn That Other Stars Are Suns? • Ancient observers didn’t think stars were like the Sun because Sun is so much brighter. • Christian Huygens (1629–1695) used holes drilled in a brass plate to estimate the angular sizes of stars. • His results showed that, if stars were like Sun, they must be at gr ...
Transit surveys for Earths in the habitable zones of white dwarfs
Transit surveys for Earths in the habitable zones of white dwarfs

... Fig. 4.— Probability density, d2 n/(dTp d log Rp ), of detected planets vs. planet radius, Rp (log axis scale), and planet effective temperature, Tp (assuming the same albedo as Earth). The contours enclose 25%, 50%, and 75% of all detected planets; the contour levels are 29%, 53%, and 76% of the pe ...
RV Metric_new_8
RV Metric_new_8

... are the planets with outcome #2, each of which has a unique probability P. We estimate the probability Pk of the kth random variable by a Monte Carlo experiment, as follows. First, we create a large sample of random values of i by drawing from the appropriate random deviate, which is arccos(1- 2Q) , ...
What is a planet? - X-ray and Observational Astronomy Group
What is a planet? - X-ray and Observational Astronomy Group

... Giordano Bruno said that the fixed stars are really suns like our own, with planets going round them • 1991 Radio astronomers Alex Wolszczan & Dale Frail discovered planets around a pulsar PSR1257+12 – Variations in arrival times of pulses suggests presence of three or more planets – Planets probabl ...
2.4 Statistical properties of radial velocity planets
2.4 Statistical properties of radial velocity planets

... and why they do not harbor planets. ...
Pluto Challenge - Cedar Amateur Astronomers
Pluto Challenge - Cedar Amateur Astronomers

... the telescope’s field of view (FOV). Stars are very, very distance objects and as a result do not move within the FOV over time. However, objects within the solar system are relatively close and always in motion around the Sun. If photographs taken at different times include solar system objects suc ...
CYGNUS CONSTELLATION, the Swan Cygnus is
CYGNUS CONSTELLATION, the Swan Cygnus is

... away. Its traditional name means "breast" and refers to its position in the constellation. Delta Cygni is another bright binary star in Cygnus, 171 light-years with a period of 800 years. The primary is a blue-white hued giant star of magnitude 2.9, and the secondary is a star of magnitude 6.6. The ...
The Sky
The Sky

... you would see many constellations and asterisms invisible from North America. – For example, the star Alpha Centauri is in the southern sky and isn’t visible from most of the United States. You could just glimpse it above the southern horizon if you were in Miami, but you could see it easily from Au ...
In This Issue The most volcanically active place is out-of- this
In This Issue The most volcanically active place is out-of- this

... We opened up the observatory a few times. I opened up HJRO a couple of times early in the morning as well to try to get a glimpse of Comet ISON. Comet LoveJoy is making an unexpected bright appearance at this time. It rivaled Ison in brightness and actually exceeded it in the middle part of November ...
Pluto and the Galactic Center
Pluto and the Galactic Center

... was demoted from being a planet to a dwarf planet. Moreover, according to this definition Ceres, the largest asteroid, is also a dwarf planet, and so is “Xena”. The IAU is also considering whether other celestial bodies beyond the orbit of Neptune (“trans-Neptunian objects”) might be classified as d ...
COMETARY PARALLAX
COMETARY PARALLAX

... object observed by amateur astronomers. This graphical method seems to favorably compare with spherical trigonometry methods (not discussed). Though applicable to some planets and our Moon, the technique will be demonstrated with comets on close approach (~1 au). This is useful for planned coordinat ...
Free floating planets
Free floating planets

... Understanding how the transiting planet mass-radius relations change as a function of orbital distance, stellar mass, stellar metallicity, or UV flux, will provide insight into the fundamentals of planetary formation, migration, and evolution. The transit method of planet detection is biased toward ...
Science Argumentative Writing Prompt Problem: Scientists have
Science Argumentative Writing Prompt Problem: Scientists have

... wind and other similar effects. After that there still may be many proto-planets orbiting the star or each other, but over time many will collide—either to form a single larger planet or release material for other larger proto-planets or planets to absorb. Some objects in space are a spherical shape ...
New Moons for Pluto!
New Moons for Pluto!

... Pluto, its moon Charon, and two other nearby objects never previously seen by other telescopes. ...
IAU-Perraut-2013 - Putting A Stars into Context
IAU-Perraut-2013 - Putting A Stars into Context

... IAU Conference « Putting A Stars into Context” Moscow, 2013 June 3rd ...
On the migration of a system of protoplanets
On the migration of a system of protoplanets

... Cochran & Mayor 1999): the 51 Peg-type planets. They all have masses of the order of MJup, and orbit their central stars very closely, having orbital periods of only a few days. As massive planets, according to standard theory, have formed at distances of ...
On the migration of a system of protoplanets
On the migration of a system of protoplanets

... Cochran & Mayor 1999): the 51 Peg-type planets. They all have masses of the order of MJup, and orbit their central stars very closely, having orbital periods of only a few days. As massive planets, according to standard theory, have formed at distances of ...
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Astronomical naming conventions

In ancient times, only the Sun and Moon, a few hundred stars and the most easily visible planets had names. Over the last few hundred years, the number of identified astronomical objects has risen from hundreds to over a billion, and more are discovered every year. Astronomers need to be able to assign systematic designations to unambiguously identify all of these objects, and at the same time give names to the most interesting objects and, where relevant, features of those objects.The International Astronomical Union (IAU) is the officially recognized authority in astronomy for assigning designations to celestial bodies such as stars, planets, and minor planets, including any surface features on them. In response to the need for unambiguous names for astronomical objects, it has created a number of systematic naming systems for objects of various sorts.
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