Communications in Asteroseismology
... is that? Mike observed all night and almost went blind measuring tiny spectra in a dark room all day. He then changed back to photometry fast! (Even though it only paid $ 16 a month.) Thus he was led (driven?) to a career in photometry. On finishing his undergraduate degree, Mike wanted to go to grad ...
... is that? Mike observed all night and almost went blind measuring tiny spectra in a dark room all day. He then changed back to photometry fast! (Even though it only paid $ 16 a month.) Thus he was led (driven?) to a career in photometry. On finishing his undergraduate degree, Mike wanted to go to grad ...
CoRoT III programme
... CoRoT specificities and how they can be optimally used to make the most relevant contribution to these scientific fields. The main asset of Kepler compared with CoRoT is the length of the light curves. It can observe quasi-continuously the same objects selected within its 100 square degrees field o ...
... CoRoT specificities and how they can be optimally used to make the most relevant contribution to these scientific fields. The main asset of Kepler compared with CoRoT is the length of the light curves. It can observe quasi-continuously the same objects selected within its 100 square degrees field o ...
Differential rotation in Sun-like stars from surface variability and
... Stellar winds: Stars like the Sun exhibit a stellar wind which consists of charged particles that are thermally and centrifugally liberated from their coronae (Parker 1958). These particles are initially locked to the magnetic field lines out to a radius where the field strength becomes less than th ...
... Stellar winds: Stars like the Sun exhibit a stellar wind which consists of charged particles that are thermally and centrifugally liberated from their coronae (Parker 1958). These particles are initially locked to the magnetic field lines out to a radius where the field strength becomes less than th ...
La Sapienza – 2015
... • So far no planets detected • Gaia space mission will measure stellar parallaxes with unprecedented precision • Gaia space mission will feature accuracy of ~30micro arc-sec • Gaia is predicted to discover 10,000 planets using astrometry in our local surrounding alone ...
... • So far no planets detected • Gaia space mission will measure stellar parallaxes with unprecedented precision • Gaia space mission will feature accuracy of ~30micro arc-sec • Gaia is predicted to discover 10,000 planets using astrometry in our local surrounding alone ...
solar system
... Sun, and a conical motion of its axis of rotation. This last motion was made necessary because Copernicus conceptualized the Earth's annual motion as the result of the Earth being embedded in a spherical shell centered on the Sun. Its axis of rotation therefore did not remain parallel to itself with ...
... Sun, and a conical motion of its axis of rotation. This last motion was made necessary because Copernicus conceptualized the Earth's annual motion as the result of the Earth being embedded in a spherical shell centered on the Sun. Its axis of rotation therefore did not remain parallel to itself with ...
Downloaded - Royal Society Open Science
... flashes’. This value of 2.0 M represents a key transition mass; the duration and character of the mass loss changes markedly when crossing this threshold. After the core helium is exhausted, a heliumburning shell is formed. At this point, the star is said to have begun evolving on the ‘asymptotic g ...
... flashes’. This value of 2.0 M represents a key transition mass; the duration and character of the mass loss changes markedly when crossing this threshold. After the core helium is exhausted, a heliumburning shell is formed. At this point, the star is said to have begun evolving on the ‘asymptotic g ...
Transit of Venus Program-Script with Image and Time Cues
... folks are not seeing the majesty of the night sky as we saw it. So, if you’ll kindly turn off the light pollution you’ll see what I mean. Ah, that’s it…just like I remember. Thank you! ...
... folks are not seeing the majesty of the night sky as we saw it. So, if you’ll kindly turn off the light pollution you’ll see what I mean. Ah, that’s it…just like I remember. Thank you! ...
Time Variation of Kepler Transits Induced By Stellar Rotating Spots
... radial-velocity signal during eclipse, as the eclipsing star moves across the disc of the eclipsed star. The RM effect is sensitive to the sky-projected component of the spin-orbit angle, and was successfully measured for many transiting planet systems (e.g., Queloz et al. 2000; Winn et al. 2006; Tr ...
... radial-velocity signal during eclipse, as the eclipsing star moves across the disc of the eclipsed star. The RM effect is sensitive to the sky-projected component of the spin-orbit angle, and was successfully measured for many transiting planet systems (e.g., Queloz et al. 2000; Winn et al. 2006; Tr ...
Analysis of Angular Momentum in Planetary Systems and Host Stars
... System’s orbital angular momentum, however, is of the same order of magnitude as the primary law, whereas the Sun’s spin angular momentum is consistent with the secondary relationship. This suggests that planets are an important clue to answering questions about stellar angular momentum loss and tra ...
... System’s orbital angular momentum, however, is of the same order of magnitude as the primary law, whereas the Sun’s spin angular momentum is consistent with the secondary relationship. This suggests that planets are an important clue to answering questions about stellar angular momentum loss and tra ...
JWST Project Report to the PMC
... 1.) Orbit that assures thermal stability and low background 2.) Orbit that assures long dwell times 3.) A stable PSF and excellent pointing 4.) Infrared sensitivity (planetary temperatures; molecules) 5.) Aperture sufficient to permit medium resolution spectroscopy These are obtained with a large ap ...
... 1.) Orbit that assures thermal stability and low background 2.) Orbit that assures long dwell times 3.) A stable PSF and excellent pointing 4.) Infrared sensitivity (planetary temperatures; molecules) 5.) Aperture sufficient to permit medium resolution spectroscopy These are obtained with a large ap ...
Maximizing the ExoEarth Candidate Yield from a Future Direct
... NASA Goddard Space Flight Center, Exoplanets & Stellar Astrophysics Laboratory, Code 667, Greenbelt, MD 20771; [email protected] ...
... NASA Goddard Space Flight Center, Exoplanets & Stellar Astrophysics Laboratory, Code 667, Greenbelt, MD 20771; [email protected] ...
Review Astronomy 1 — Elementary Astronomy LA Mission College Spring F2015
... “One may wonder, What came before? If space-time did not exist then, how could everything appear from nothing? . . . Explaining this initial singularity—where and when it all began—still remains the most intractable problem of modern cosmology. — Andrei Linde “But who shall dwell in these worlds if ...
... “One may wonder, What came before? If space-time did not exist then, how could everything appear from nothing? . . . Explaining this initial singularity—where and when it all began—still remains the most intractable problem of modern cosmology. — Andrei Linde “But who shall dwell in these worlds if ...
Halley`s Comet Strikes Back!
... {{Information |Description={{en|1=Bill Haley and his Comets during a TV-appearance.}} {{de|1=Bill Haley and his Comets während eines Fernsehauftrittes.}} |Source=This image was provided with the friendly permission by Mr. Klau Klettner from Hydra Records {{Information |Description=Comet 17P/Holmes 1 ...
... {{Information |Description={{en|1=Bill Haley and his Comets during a TV-appearance.}} {{de|1=Bill Haley and his Comets während eines Fernsehauftrittes.}} |Source=This image was provided with the friendly permission by Mr. Klau Klettner from Hydra Records {{Information |Description=Comet 17P/Holmes 1 ...
Proposal - ESA Science
... exoplanets and relate this directly to the type and chemical environment of the host star. For this ambitious scientific programme, ARIEL is designed as a dedicated survey mission for transit and eclipse spectroscopy, capable of observing a large and well-defined planet sample within its 3.5-year mi ...
... exoplanets and relate this directly to the type and chemical environment of the host star. For this ambitious scientific programme, ARIEL is designed as a dedicated survey mission for transit and eclipse spectroscopy, capable of observing a large and well-defined planet sample within its 3.5-year mi ...
azu_etd_13224_sip1_m
... wanted during this time. I was also supported during the summer by Dr. Griffith’s NASA’s Planetary Atmospheres Program grant, and during this last year by a NASA Keck PI grant. In addition, my thesis was possible due to the data available in the Keck Observatory Archive (KOA), operated by the W. M. ...
... wanted during this time. I was also supported during the summer by Dr. Griffith’s NASA’s Planetary Atmospheres Program grant, and during this last year by a NASA Keck PI grant. In addition, my thesis was possible due to the data available in the Keck Observatory Archive (KOA), operated by the W. M. ...
Dynamical evolution of planetary systems
... There are two possible mechanisms by which we envision that giant planets can form. The first is nicknamed the “core-accretion mechanism”: the coagulation of solid particles forms a core typically of about 10 Earth masses (M⊕ ) while the gas is still present in the proto-planetary disk; the core the ...
... There are two possible mechanisms by which we envision that giant planets can form. The first is nicknamed the “core-accretion mechanism”: the coagulation of solid particles forms a core typically of about 10 Earth masses (M⊕ ) while the gas is still present in the proto-planetary disk; the core the ...
2009 THE INTERNATIONAL YEAR OF ASTRONOMY
... Contents IYA 2009 The background Pythagoras and the dawn of science The geocentric model The Copernican revolution ...
... Contents IYA 2009 The background Pythagoras and the dawn of science The geocentric model The Copernican revolution ...
M sin i
... massive body. But the Sun also orbits around this barycenter. – Note that Jupiter has contains more than double the mass of all the other planets together. Jupiter moves the Sun with an amplitude of A = 12.5 m/s and a period of P = 12 yr. For Saturn A = 2.7 m/s, and P = 30 yr. Nowadays the search is ...
... massive body. But the Sun also orbits around this barycenter. – Note that Jupiter has contains more than double the mass of all the other planets together. Jupiter moves the Sun with an amplitude of A = 12.5 m/s and a period of P = 12 yr. For Saturn A = 2.7 m/s, and P = 30 yr. Nowadays the search is ...
abstracts book - Instituto de Astrofísica e Ciências do Espaço
... has secured major advances in the understanding of the physics of the stellar interiors and has allowed us to build and prepare the tools to look at other stars. Several ground facilities and space missions have completed the picture by adding the necessary data to study stars across the HR diagram ...
... has secured major advances in the understanding of the physics of the stellar interiors and has allowed us to build and prepare the tools to look at other stars. Several ground facilities and space missions have completed the picture by adding the necessary data to study stars across the HR diagram ...
Worlds Beyond: A Strategy for the Detection and Characterization of
... so bright sun-like stars in the mid-term is space-based astrometry, and this is one cornerstone of the Task Force recommendations. To study the planet atmosphere for signs of habitability or life, direct imaging is required, and the Task Force Report recommends investment in direct imaging technolog ...
... so bright sun-like stars in the mid-term is space-based astrometry, and this is one cornerstone of the Task Force recommendations. To study the planet atmosphere for signs of habitability or life, direct imaging is required, and the Task Force Report recommends investment in direct imaging technolog ...
Looking for planets with SPHERE in planetary systems with double
... In most cases, the only planet of the system would have been detected and, as far as actually it has not been found, we moved to analyze multi-planetary models. ...
... In most cases, the only planet of the system would have been detected and, as far as actually it has not been found, we moved to analyze multi-planetary models. ...
Tidal Venuses: Triggering a Climate Catastrophe via Tidal Heating
... i.e. one hemisphere always facing the star, was emphasized. Kasting et al. (1993) quantified this concept and found that planets orbiting within the HZ of stars less than two-thirds the mass of the Sun were in danger of synchronization. Although their analysis was limited to Earth-like planets on ci ...
... i.e. one hemisphere always facing the star, was emphasized. Kasting et al. (1993) quantified this concept and found that planets orbiting within the HZ of stars less than two-thirds the mass of the Sun were in danger of synchronization. Although their analysis was limited to Earth-like planets on ci ...
ABSTRACT Exoplanet Habitability and an Analysis of Gliese 436 b
... activity.12 The amount of variation in temperature between the two extremes of this cycle greatly affects if an exoplanet can sustain the conditions necessary for life. What is important to note about all these different factors for life to exist is that it takes very precise ranges of multiple vari ...
... activity.12 The amount of variation in temperature between the two extremes of this cycle greatly affects if an exoplanet can sustain the conditions necessary for life. What is important to note about all these different factors for life to exist is that it takes very precise ranges of multiple vari ...
SPIRou Science Case
... One of the most exciting areas of astronomical research today is the study of exoplanets & exoplanetary systems, engaging the imagination not just of the astronomical community but of the general population. Since the pioneering discovery of a giant planet around 51 Peg (Mayor & Queloz 1995, Nature ...
... One of the most exciting areas of astronomical research today is the study of exoplanets & exoplanetary systems, engaging the imagination not just of the astronomical community but of the general population. Since the pioneering discovery of a giant planet around 51 Peg (Mayor & Queloz 1995, Nature ...
Kepler (spacecraft)
Kepler is a space observatory launched by NASA to discover Earth-like planets orbiting other stars. The spacecraft, named after the German Renaissance astronomer Johannes Kepler, was launched on March 7, 2009.Designed to survey a portion of our region of the Milky Way to discover dozens of Earth-size extrasolar planets in or near the habitable zone and estimate how many of the billions of stars in the Milky Way have such planets, Kepler's sole instrument is a photometer that continually monitors the brightness of over 145,000 main sequence stars in a fixed field of view. This data is transmitted to Earth, then analyzed to detect periodic dimming caused by extrasolar planets that cross in front of their host star.Kepler is part of NASA's Discovery Program of relatively low-cost, focused primary science missions. The telescope's construction and initial operation were managed by NASA's Jet Propulsion Laboratory, with Ball Aerospace responsible for developing the Kepler flight system. The Ames Research Center is responsible for the ground system development, mission operations since December 2009, and scientific data analysis. The initial planned lifetime was 3.5 years, but greater-than-expected noise in the data, from both the stars and the spacecraft, meant additional time was needed to fulfill all mission goals. Initially, in 2012, the mission was expected to last until 2016, but this would only have been possible if all remaining reaction wheels used for pointing the spacecraft remained reliable. On May 11, 2013, a second of four reaction wheels failed, disabling the collection of science data and threatening the continuation of the mission.On August 15, 2013, NASA announced that they had given up trying to fix the two failed reaction wheels. This meant the current mission needed to be modified, but it did not necessarily mean the end of planet-hunting. NASA had asked the space science community to propose alternative mission plans ""potentially including an exoplanet search, using the remaining two good reaction wheels and thrusters"". On November 18, 2013, the K2 ""Second Light"" proposal was reported. This would include utilizing the disabled Kepler in a way that could detect habitable planets around smaller, dimmer red dwarfs. On May 16, 2014, NASA announced the approval of the K2 extension.As of January 2015, Kepler and its follow-up observations had found 1,013 confirmed exoplanets in about 440 stellar systems, along with a further 3,199 unconfirmed planet candidates. Four planets have been confirmed through Kepler 's K2 mission. In November 2013, astronomers reported, based on Kepler space mission data, that there could be as many as 40 billion Earth-sized planets orbiting in the habitable zones of Sun-like stars and red dwarfs within the Milky Way. It is estimated that 11 billion of these planets may be orbiting Sun-like stars. The nearest such planet may be 3.7 parsecs (12 ly) away, according to the scientists.On January 6, 2015, NASA announced the 1000th confirmed exoplanet discovered by the Kepler Space Telescope. Four of the newly confirmed exoplanets were found to orbit within habitable zones of their related stars: three of the four, Kepler-438b, Kepler-442b and Kepler-452b, are near-Earth-size and likely rocky; the fourth, Kepler-440b, is a super-Earth.