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Neptunus
Neptunus

... atmospheric pressure. The mostly water-ice surface has many large cracks, probably caused by partial melting of the interior, and ice geysers spew nitrogen gas and dark, presumably carbon-rich particles several miles into the thin atmosphere. Winds then blow the gas sideways, forming dark plumes. In ...
EVOLUTIONARY TRACKS OF THE CLIMATE OF EARTH
EVOLUTIONARY TRACKS OF THE CLIMATE OF EARTH

... age may change from 0.6 to 4.4 Gyr. It is, however, noted that the characteristic features obtained from this study do not change in the cases with different parameter values: the duration for a hypothetical Earth to have a warm climate similar to the present Earth is very limited, even though the p ...
Astronomy From Å to ZZ — Howard L. Cohen
Astronomy From Å to ZZ — Howard L. Cohen

... James Walter Christy discovered Charon in 1978 at the Naval Observatory from a slight elongation or “bump” in a photograph of Pluto. Charon is named for the mythical ferryman who conveyed the dead to Hades over the river Styx. (Pluto was the Roman god of the dead and ruler of the underworld.) Charon ...
Reading Earth in Space
Reading Earth in Space

... 2. Find sentences in the text that mean the same: Tycho Brahe said he was better at mathematics than another boy. The boy broke a part of his body. He started to be interested in Astronomy after a solar phenomenon. Brahe used a big instrument to see where a new star was. A monarch gave Brahe a place ...
File
File

... Describe the methods scientists have used to help with this search in both our Solar System and the rest of the Universe. ...
Stars
Stars

... d. spectrum. ______ 6. A hot, solid object gives off a(n) a. continuous spectrum. b. absorption spectrum. c. emission line. d. partial spectrum. ______ 7. What colors are shown in a continuous spectrum? a. primary colors b. cool colors c. warm colors d. all colors ...
Integrative Studies 410 Our Place in the Universe
Integrative Studies 410 Our Place in the Universe

... Stage 13: White Dwarf • Core radiates only by stored heat, not by nuclear reactions • core continues to cool and contract • Size ~ Earth • Density: a million times that of Earth – 1 cubic cm has 1000 kg of mass! ...
Howard 2013 Observed properties of exoplanets
Howard 2013 Observed properties of exoplanets

... 2700 planet candidates (3–5), of which only 5 to 10% are likely to be false-positive detections (6, 7). Giant planets in more distant orbits have also been detected through imaging (8) and gravitational microlensing surveys (9). With the Doppler technique, planet masses and orbits are inferred from ...
Lecture 1
Lecture 1

... Occasionally you misunderstand a question that a student asks and answer with a completely unrelated explanation. I can usually identify what you thought the question was and what you're explaining but I feel like most students are often confused. When we discussed bias in terms of practical example ...
Are You Smarter... Review Game
Are You Smarter... Review Game

... classify the planets as either inner or outer! The Inner planets consist of Mercury, Venus, Earth and Mars. The Outer planets consist Jupiter, Saturn, Uranus, and Neptune. We also call the Inner planets terrestrial planets, and the Outer planets gas giants. ...
Astronomy (stars, galaxies and the Universe)
Astronomy (stars, galaxies and the Universe)

... All stars are created from the gases in a nebula When the contracting gas and dust from a nebula become so dense and hot that nuclear fusion begins, the protostar begins to shine When a star begins to run out of fuel, its core shrinks and its outer portion expands The evolutionary path of a star dep ...
February - Bristol Astronomical Society
February - Bristol Astronomical Society

... Batista Hodierna around 1654, it was probably quite well known to ancient astronomers. Charles Messier, was one of many people who later rediscovered the cluster. He added it to his famous catalogue on January 16, 1765 ...
Proposal submitted to ISSI
Proposal submitted to ISSI

... project are important for discovery missions such as CoRoT, which may detect remnants of “Hot Jupiters”, “Hot Neptunes”, and Super Earths”, and Kepler and SIM, hunting for Earth-sized planets. Moreover the proposed results are crucial for understanding the evolution of planetary atmospheres within t ...
Ch 28-31 Lessons
Ch 28-31 Lessons

... 2. What force causes Earth’s mass to move outward from its center at the equator as Earth rotates on its axis? ________________________________________________________________ 3. Where is the… a. … slight bulging of Earth’s circumference? the equator or the poles b. … slight squishing of Earth’s cir ...
Is there life in space? Activity 2: Moving Stars and Their Planets
Is there life in space? Activity 2: Moving Stars and Their Planets

... Q. Most of the planets that have been discovered orbit their stars at a tilt closer to 0 degrees than to 90 degrees. Why? A. The signal is more evident when the tilt is lower. The telescopes are not perfect, so they can only detect star motions that are very large. The largest motions occur when the ...
Environmental Science
Environmental Science

... Over the course of time, the North Star changes. Right now Polaris is within one degree of true north, but at other times the North Star has been and will again be Thuban (the brightest star in the constellation Draco), Vega (the brightest star in the constellation Lyra), and Alpha Cephei (the brigh ...
Precession of Earth
Precession of Earth

... Over the course of time, the North Star changes. Right now Polaris is within one degree of true north, but at other times the North Star has been and will again be Thuban (the brightest star in the constellation Draco), Vega (the brightest star in the constellation Lyra), and Alpha Cephei (the brigh ...
WFIRST-2.4: What Every Astronomer Should Know
WFIRST-2.4: What Every Astronomer Should Know

... In response to this opportunity, NASA commissioned a new SDT to create a design reference mission for WFIRST using one of these 2.4m telescopes. This short article describes the highlights of this DRM, hereafter referred to as WFIRST-2.4, and serves as an entry point to the much more detailed descri ...
9J Gravity and Space
9J Gravity and Space

... (HST), are large telescopes placed in a high orbit far from the effects of the Earth’s atmosphere. These satellites can ‘see’ much further into space and give us images of stars and galaxies many light years away, like this cartwheel galaxy. ...
9J Gravity and Space - We can`t sign you in
9J Gravity and Space - We can`t sign you in

... (HST), are large telescopes placed in a high orbit far from the effects of the Earth’s atmosphere. These satellites can ‘see’ much further into space and give us images of stars and galaxies many light years away, like this cartwheel galaxy. ...
1 Lecture 8: Uranus and Neptune
1 Lecture 8: Uranus and Neptune

... – theoretical models suggest that Neptune has a rocky core similar to Jupiter and Saturn (about 10 earth masses) – rocky core of Uranus makes up a large fraction of the planet as compared to Jupiter and Saturn – pressure outside the core too low to form metallic hydrogen – origin of the magnetic fie ...
Ch 20 Notes Stars
Ch 20 Notes Stars

... • When a scientist observes a galaxy that is 1 billion years away, they are observing light that left the galaxy 1 billion years ago • Scientists don’t know what the galaxy looks like now, but can study similar closer galaxies to piece together the evolution of galaxies • The gas, dust and stars tha ...
Diapositiva 1
Diapositiva 1

... nebulae have long been appreciated as a final phase in the life of a sunlike star. Only much more recently however, have some planetaries been found to have halos like this one, likely formed of material shrugged off during earlier active episodes in the star's evolution. While the planetary nebula ...
Gravity - Indiana University Astronomy
Gravity - Indiana University Astronomy

... Discuss with a partner what assumptions might be reasonable for scientists to make about the Universe. List three or four. For each describe why this is a reasonable assumption for our universe, and what the assumptions might imply for the origin, evolution, or structure of our universe. a) ...
Volume 1 (Issue 6), June 2012
Volume 1 (Issue 6), June 2012

... Mercury, accordingly are the planets for which we see transits. However, as seen from outer planets such as Mars, Jupiter etc, the Earth itself transits the Sun. While transits of Mercury are relatively common, occurring once or twice every decade, the transits of Venus are extremely rare, occurring ...
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Extraterrestrial life



Extraterrestrial life is life that does not originate from Earth. It is also called alien life, or, if it is a sentient and/or relatively complex individual, an ""extraterrestrial"" or ""alien"" (or, to avoid confusion with the legal sense of ""alien"", a ""space alien""). These as-yet-hypothetical life forms range from simple bacteria-like organisms to beings with civilizations far more advanced than humanity. Although many scientists expect extraterrestrial life to exist, so far no unambiguous evidence for its existence exists.The science of extraterrestrial life is known as exobiology. The science of astrobiology also considers life on Earth as well, and in the broader astronomical context. Meteorites that have fallen to Earth have sometimes been examined for signs of microscopic extraterrestrial life. Since the mid-20th century, there has been an ongoing search for signs of extraterrestrial intelligence, from radios used to detect possible extraterrestrial signals, to telescopes used to search for potentially habitable extrasolar planets. It has also played a major role in works of science fiction. Over the years, science fiction works, especially Hollywood's involvement, has increased the public's interest in the possibility of extraterrestrial life. Some encourage aggressive methods to try to get in contact with life in outer space, whereas others argue that it might be dangerous to actively call attention to Earth.
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