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Cosmology Astrophysics Astronomy
Latest Activity: on Friday
Cosmology - Astrophysics - Astronomy
Hubble Wallpaper - Awesome Hubble Images
Started by Tom Sarbeck. Last reply by Joey Daniel Smith Dec 22, 2018.
Started by Mrs.B. Last reply by Mrs.B Apr 9, 2016.
Started by Davy. Last reply by Onyango Makagutu Mar 8, 2016.
Started by Davy Oct 3, 2013.
Started by Davy. Last reply by Davy Aug 15, 2013.
Explanation: The largest canyon in the Solar System cuts a wide swath across the face of Mars. Named Valles Marineris, the grand valley extends over 3,000 kilometers long, spans as much as 600 kilometers across, and delves as much as 8 kilometers deep. By comparison, the Earth's Grand Canyon in Arizona, USA is 800 kilometers long, 30 kilometers across, and 1.8 kilometers deep. The origin of the Valles Marineris remains unknown, although a leading hypothesis holds that it started as a crack billions of years ago as the planet cooled. Several geologic processes have been identified in the canyon. The above mosaic was created from over 100 images of Mars taken by Viking Orbiters in the 1970s.
yet another amazing video from the link off of Radu's page:
i just swiped this awesome video off of Radu's page, fascinating, i smiled all the way from first moment to last:
WOW! Sun Eruption Creates Spectacular Plasma Tentacle
A NASA spacecraft watching the sun has caught a dazzling view of a solar eruption that launched a vast tendril of magnetic plasma into space.
NASA's Solar Dynamics Observatory recorded the sun tentacle, which scientists call a solar prominence, on March 19 as it erupted into space with a rounded, twisting motion.
The eruption occurred over five hours as SDO watched the sun in the ultraviolet range of the light spectrum, SDO mission scientists said in a statement. The solar observatory watched as the prominence twisted up from the sun and expanded, then became unstable. [Video: Round Eruption From the Sun]
Ultimately, the sun filament lost cohesion and its particles streamed away from the sun.
"Prominences are elongated clouds of plasma that hover above the sun's surface, tethered by magnetic forces," SDO mission scientists explained.
The sun is currently in the midst of an active phase of its 11-year solar weather cycle and has kicked up a series of powerful eruptions and flares in recent months. The SDO spacecraft and other space observatories are keeping a close watch on the sun to monitor is solar weather activity. [Amazing Sun Photos from Space]
Earlier this month, the sun unleashed its second X-class solar flare of the year that was aimed at Earth. X-class solar flares are the strongest types of solar flares. The weakest types of solar flares are Class C sun storms, with Class M flares registering as medium strength, but still powerful, NASA scientists have said.
Strong solar flares, when aimed at Earth, can potentially disrupt satellites and power grids, as well as pose a hazard to astronauts on spacecraft. They can also spark dazzling shows of the northern lights, or aurora borealis.
From Starts with a Bang
Except, that is, near the North and South magnetic poles, where those field lines all appear to enter/exit our planet. And whenever the Sun emits a flare, prominence, or other "event," here's what happens.
(Image credit: NASA's Marshall Space Flight Center.)
Eye Candy: The Square Nebula
DEEP SPACE - Brown dwarf could be coldest known starCBC News Posted: Mar 23, 2011 10:23 AM ETAstronomers say they've found a new candidate for the coldest known star — a brown dwarf with the temperature of a freshly made cup of tea.While you might burn yourself drinking such a tea, at 100 degrees Celsius, the boiling point of water is actually extremely cold for the surface of a star. The temperature of Earth's sun, for example, is about 5,500 C.Scientists liken brown dwarfs to failed stars because they aren't big enough for gravity to trigger the nuclear reactions that make stars shine. Astronomers say such discoveries are significent because a brown dwarf is not exactly a star and not exactly a planet, but instead something between the two, and hence can teach us about the physics of both.Working with the European Southern Observatory's Very Large Telescope, astronomers say the newly-discovered brown dwarf is one of a pair in a double system 75 light-years from Earth. Astronomers describe the brown dwarfs, identified as CFBDSIR 1458+10B, in a paper in the current issue of The Astrophysical Journal."At such temperatures we expect the brown dwarf to have properties that are different from previously known brown dwarfs and much closer to those of giant exoplanets — it could even have water clouds in its atmosphere," the paper's lead author, Michael Liu of the University of Hawaii's Institute for Astronomy, said in a release.The team of researchers, which included Etienne Artigau of the Université de Montréal, is not ready to say it has definitively found the coldest known star.That's because another team working with NASA's infrared Spitzer Space Telescope recently identified two other very faint objects as other possible candidates, although their temperatures have not yet been measured so precisely.
This artist's impression shows the pair of brown dwarfs named CFBDSIR 1458+10. They are the coolest pair of brown dwarfs found so far. The colder of the two components (shown in the background) is a candidate for the brown dwarf with the lowest temperature ever found. (L. Calcada/ESO)
Testing gravity in gas-rich galaxies
Karen Masters & Kristine SpekkensThe rotation curve of a galaxy is the orbital speed of material as a function of distance from the center of the galaxy. In the 1970s, the astronomer Vera Rubin measured the rotation curves of several of the nearest spiral galaxies. To her astonishment, the curves remained flat beyond the edge of the galaxy’s stellar disc . Under the standard theory of gravity this implies that the mass in the outskirts of these systems far outweighs that of the detected gas and stars. Today, the flatness of spiral galaxy rotation curves remains key evidence for dark matter, which, broadly defined, is matter that obeys the law of gravity but does not emit any light.Dark matter is an integral component of the currently favored cosmological model, in which over 90% of the matter in the Universe is made up of massive (“cold”) particles, which interact only via gravity. The model is named Lambda-Cold Dark Matter (ΛCDM), with Λ denoting a cosmological constant (sometimes called “dark energy”) that accelerates expansion at late cosmological times. An impressive array of observations fit this picture, from the spectrum of fluctuations in the cosmic microwave background (the first free-streaming photons in the Universe, e.g., Ref. ), to the luminosities of distant supernovae. The astrophysical community has adopted ΛCDM as the standard cosmological model, which makes the nature of dark matter one of the most important outstanding questions in the field.But not all cosmologists are happy with this picture. Some are uneasy with the unknown components in the standard model, and worry that cosmology in the last 30 years has degraded into “naming the unknown” . In spiral galaxies at least, an alternative to invoking dark matter is to modify the theory of gravity in regions where there is a discrepancy between the mass inferred from dynamics (using standard gravity) and the baryonic mass (i.e., the census of normal material detected in stars and gas). The most successful of these ideas is MOND (Modified Newtonian Dynamics ), which modifies gravity at small accelerations to produce flat galactic rotation curves. For gravitational accelerations a less than some critical value a0, the usual Newtonian relation F=ma is modified to F=ma2/a0, and therefore the circular velocity around a mass M asymptotes to a constant value vf=(GMa0)1/4. Once the universal constant a0 is fixed observationally, MOND explains the rotation curve shapes of galaxies using their baryonic mass alone, while simultaneously accounting for the observed correlation between their rotation velocities and luminosities.Read more here from Physics.Via our Library/More... resource pages.
Explanation: Did you see the Full Moon last night? Near the horizon, the lunar orb may have seemed to loom large, swollen in appearance by the famous Moon illusion. But the Full Moon really was a large Full Moon last night, reaching its exact full phase within an hour of lunar perigee, the point in the Moon's elliptical orbit closest to planet Earth. A similar near perigee Full Moon last occured on December 12, 2008. The difference in the Moon's apparent size as it moves from perigee to apogee, its farthest point from Earth, is about 14 percent. Of course, a nearly Full Moon will rise again tonight, lighting the skies on the date of the Equinox or equal night. The Full Moon also looms large in this well-planned, telescopic lunar portrait. Captured earlier this year, the rising lunar orb is dramatically matched to the 2,500 year old Parthenon, in Athens, Greece.
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