![Libra (constellation)](http://s1.studyres.com/store/data/000501688_1-83bb74ae05270b9beb5572a404f86223-300x300.png)
Libra (constellation)
... σ Librae was formerly known as γ Scorpii despite being well inside the boundaries of Libra. It was not redesignated as σ Librae until 1851 (by Benjamin A. Gould). ...
... σ Librae was formerly known as γ Scorpii despite being well inside the boundaries of Libra. It was not redesignated as σ Librae until 1851 (by Benjamin A. Gould). ...
Giant Planet Formation
... giant planets • Stars with one detectable giant planet are more likely to host more detectable planets • > a few % of stars have Jupiter-like companions (0.5 - 2 MJup, 4 AU < a < 7 AU), but > 25% do not • Brown dwarf desert; Jupiter-mass planets most common giants ...
... giant planets • Stars with one detectable giant planet are more likely to host more detectable planets • > a few % of stars have Jupiter-like companions (0.5 - 2 MJup, 4 AU < a < 7 AU), but > 25% do not • Brown dwarf desert; Jupiter-mass planets most common giants ...
PLANETS
... Substantial eccentricity of many of the orbits. No clear answers to either of these surprises, but lots of ideas... ...
... Substantial eccentricity of many of the orbits. No clear answers to either of these surprises, but lots of ideas... ...
RV metric 2
... which could spectroscopically characterize their atmospheres or surfaces in reflected starlight. To help differentiate mission concepts, and to help develop reasonable scientific expectations, we propose a science metric for RV exoplanets. This metric is the estimated number of such planets detected ...
... which could spectroscopically characterize their atmospheres or surfaces in reflected starlight. To help differentiate mission concepts, and to help develop reasonable scientific expectations, we propose a science metric for RV exoplanets. This metric is the estimated number of such planets detected ...
The Planetary bodies
... The main issue is that none of us come into this realm at the exact placements of all these planetary bodies, as they are working together. Example: If you are a Virgo with a Virgo ascendant, it wont carry the same energy as Aries in the first house. Instead Virgo brings the analytical side to the f ...
... The main issue is that none of us come into this realm at the exact placements of all these planetary bodies, as they are working together. Example: If you are a Virgo with a Virgo ascendant, it wont carry the same energy as Aries in the first house. Instead Virgo brings the analytical side to the f ...
Extrasolar Planets
... In 2004, a planet oneand-a-half times more massive than Jupiter was discovered orbiting a red dwarf star 17,000 light years away. This marks the first discovery of an extrasolar planet using gravitational microlensing. ...
... In 2004, a planet oneand-a-half times more massive than Jupiter was discovered orbiting a red dwarf star 17,000 light years away. This marks the first discovery of an extrasolar planet using gravitational microlensing. ...
Test - Scioly
... 11) Alinda Asteroids also have a 4:1 resonance ratio with Earth. These asteroids come close to Earth how many years? 12) Scattered Disk Objects come in gravitational range within which planet? 13) Neptune’s outer layer is composed of what element? ...
... 11) Alinda Asteroids also have a 4:1 resonance ratio with Earth. These asteroids come close to Earth how many years? 12) Scattered Disk Objects come in gravitational range within which planet? 13) Neptune’s outer layer is composed of what element? ...
to view poster PDF
... ・Rare atmosphere extends out to several planetary radii ・Mass loss from atmosphere ☆Mass loss from hot Jupiter can be detected by using transit method ...
... ・Rare atmosphere extends out to several planetary radii ・Mass loss from atmosphere ☆Mass loss from hot Jupiter can be detected by using transit method ...
lec13_05nov2007
... attributed to formation by core accretion • RV searches are beginning to find planets around low [Fe/H] dwarfs (HD 155358: [Fe/H] = -0.68 has two planets with masses of 0.5 and 0.9 MJup, Cochran et al. 2007; HD 171028: [Fe/H] = -0.49 has one with 1.8 MJup, ...
... attributed to formation by core accretion • RV searches are beginning to find planets around low [Fe/H] dwarfs (HD 155358: [Fe/H] = -0.68 has two planets with masses of 0.5 and 0.9 MJup, Cochran et al. 2007; HD 171028: [Fe/H] = -0.49 has one with 1.8 MJup, ...
Search for Life in the Universe
... Solar System Formation • Standard theory: Jovian planets form at large distances ~ 5 AU and more • So why are they closer? • Theory of planet formation wrong? – We have not found a flaw, even when looking hard after the discovery of the extrasolar planets ...
... Solar System Formation • Standard theory: Jovian planets form at large distances ~ 5 AU and more • So why are they closer? • Theory of planet formation wrong? – We have not found a flaw, even when looking hard after the discovery of the extrasolar planets ...
The (Super)Wasp Factory Finds 10 New Planets In The Last 6 Months
... 45 planets have now been discovered using the transit method, and since they started operation in 2004 the SuperWASP cameras have found 15 of them – making them by far the most successful discovery instruments in the world. The SuperWASP planets have masses between a middleweight 0.5 and a huge 8.3 ...
... 45 planets have now been discovered using the transit method, and since they started operation in 2004 the SuperWASP cameras have found 15 of them – making them by far the most successful discovery instruments in the world. The SuperWASP planets have masses between a middleweight 0.5 and a huge 8.3 ...
radioactive age dating
... depends in part on its composition • An object sinks in a fluid if its average density is greater than that of the fluid, but rises if its average density is less than that of the fluid • The terrestrial (inner) planets are made of rocky materials and have dense iron cores, which gives these planets ...
... depends in part on its composition • An object sinks in a fluid if its average density is greater than that of the fluid, but rises if its average density is less than that of the fluid • The terrestrial (inner) planets are made of rocky materials and have dense iron cores, which gives these planets ...
Key Stage 3 – Perfect planet
... Exoplanet information: Gliese-581g Planet hunters announced the discovery of Gliese-581g in 2010. The find was the result of more than ten years of observations using one of the world’s biggest telescopes. Its parent star, Gliese-581, is a red giant. It is in the constellation Libra, and is about 20 ...
... Exoplanet information: Gliese-581g Planet hunters announced the discovery of Gliese-581g in 2010. The find was the result of more than ten years of observations using one of the world’s biggest telescopes. Its parent star, Gliese-581, is a red giant. It is in the constellation Libra, and is about 20 ...
Gravity and Orbits - Classical Physics / Santurri
... https://phet.colorado.edu/sims/html/gravity-and-orbits/latest/gravity-and-orbits_en.html ...
... https://phet.colorado.edu/sims/html/gravity-and-orbits/latest/gravity-and-orbits_en.html ...
Indirect
... • Virtually impossible to directly photograph (and therefore detect) a planet around any other star! – Think back to your “scale model solar system” homework assignment… – Imagine trying to see a 2 mm-sized “Earth” orbiting another “basketball” that is 4000 miles away! Especially if the “basketball” ...
... • Virtually impossible to directly photograph (and therefore detect) a planet around any other star! – Think back to your “scale model solar system” homework assignment… – Imagine trying to see a 2 mm-sized “Earth” orbiting another “basketball” that is 4000 miles away! Especially if the “basketball” ...
Document
... Extrasolar Planetary Science Extrasolar Planets are planets orbiting around main sequence stars other than the Sun. ...
... Extrasolar Planetary Science Extrasolar Planets are planets orbiting around main sequence stars other than the Sun. ...
"Sam`s Voyage Ends" TEST
... Fill in the Blank (1 point each) 10. _________________ - spinning round and round. 11. ________________ -largest object you can see in the night sky. 12. ________________________________- ball of hot gases 13. ______________________- light and heat from the sun. 14. _______________________________-l ...
... Fill in the Blank (1 point each) 10. _________________ - spinning round and round. 11. ________________ -largest object you can see in the night sky. 12. ________________________________- ball of hot gases 13. ______________________- light and heat from the sun. 14. _______________________________-l ...
radioactive age dating
... direction, and all of their orbits are in nearly the same plane 3. The terrestrial planets orbit close to the Sun, while the Jovian planets orbit far from the Sun ...
... direction, and all of their orbits are in nearly the same plane 3. The terrestrial planets orbit close to the Sun, while the Jovian planets orbit far from the Sun ...
ExtraSolar Planets – Student Guide
... technique. What types of planets is it effective at finding? ...
... technique. What types of planets is it effective at finding? ...
Neptune Trojans
... - If formed in current location must have initially been on circular orbit (Stern 2005). - If interacted with currently known giant planets its perihelion must have been raised some how. ...
... - If formed in current location must have initially been on circular orbit (Stern 2005). - If interacted with currently known giant planets its perihelion must have been raised some how. ...
ExtraSolar Planets – Student Guide
... You have been running an observing program hunting for extrasolar planets in circular orbits using the radial velocity technique. Suppose that all of the target systems have inclinations of 90°, stars with a mass of 1.0 Msun, and no eccentricity. Your program has been in operation for 8 years and yo ...
... You have been running an observing program hunting for extrasolar planets in circular orbits using the radial velocity technique. Suppose that all of the target systems have inclinations of 90°, stars with a mass of 1.0 Msun, and no eccentricity. Your program has been in operation for 8 years and yo ...
MS Word version
... You have been running an observing program hunting for extrasolar planets in circular orbits using the radial velocity technique. Suppose that all of the target systems have inclinations of 90°, stars with a mass of 1.0 Msun, and no eccentricity. Your program has been in operation for 8 years and yo ...
... You have been running an observing program hunting for extrasolar planets in circular orbits using the radial velocity technique. Suppose that all of the target systems have inclinations of 90°, stars with a mass of 1.0 Msun, and no eccentricity. Your program has been in operation for 8 years and yo ...
Super-Earth
![](https://commons.wikimedia.org/wiki/Special:FilePath/Exoplanet_Comparison_CoRoT-7_b.png?width=300)
A super-Earth is an extrasolar planet with a mass higher than Earth's, but substantially below the mass of the Solar System's ice giants Uranus and Neptune, which are 15 and 17 Earth masses respectively. The term super-Earth refers only to the mass of the planet, and does not imply anything about the surface conditions or habitability. The alternative term ""gas dwarfs"" may be more accurate for those at the higher end of the mass scale, as suggested by MIT professor Sara Seager, although mini-Neptunes is more common.