»
  Night Sky Calendar - Southern Hemisphere
July 2008
Celestial Object
 


04 - Earth at aphelion (farthest from Sun) at 8h UT. The Sun - Earth distance
0000is 1.01675 a.u. or about 152.1 million km.
06 - Moon near Mars at 16h UT (evening sky). Mag. +1.7.
16 - Moon near Saturn at 20h UT (evening sky). Mag. +0.8.
19 - Jupiter at opposition at 8h UT (mag. -2.7). Bes time to observe the largest
0000planet in in the solar system.
10 - Mars 0.64 from Saturn at 16h UT (47° from Sun, evening sky) Mag.+1.7 & +0.8.
17 - Moon near Jupiter at 14h UT (midnight sky). Mag. -2.7.
18 - Full Moon at 7:59 UT. The full moon of July is called the "Thunder Moon"
0000or "Hay Moon" .
29 - Mercury at superior conjunction at 20h UT (not visible). Passes into the evening sky.

00 0 0 0 0 0// Get the complete calendar version at skymaps.com
7 -

The photo was taken by the Hubble Space Telescope and shows a detail of the nebula. This close-up shows a dense cloud of dust and gas, a stellar nursery full of embryonic stars. This cloud is about 8 light-years away from the nebula's central star, not shown in this picture. Located in Sagitarius, the nebula's name means "divided into three lobes".
»
 
  Featured Book ~ The Outrageous Tales of a Space Shuttle Astronaut | Mike Mullane
The Outrageous Tales of a Space Shuttle AstronautThe Outrageous Tales of a Space Shuttle Astronaut - On February 1, 1978, the first group of space shuttle astronauts, twenty-nine men and six women, were introduced to the world. Among them would be history makers, including the first American woman and the first African American in space. This assembly of astronauts would carry NASA through the most tumultuous years of the space shuttle program. Four would die on Challenger. Mullane vividly portrays every aspect of the astronaut experience -- from telling a female technician which urine-collection condom size is a fit; to walking along a Florida beach in a last, tearful goodbye with a spouse; to a wild, intoxicating, terrifying ride into space; to hearing "Taps" played over a friend's grave. Mullane is brutally honest in his criticism of a NASA leadership whose bungling would precipitate the Challenger disaster.  


 


Saturday, October 28, 2006

Image Credit: ESA/NASA

Hubble has returned to the intriguing variable star V838 Monocerotis many times since its initial outburst in 2002, to follow the evolution of its light echo. Two new images provide the most astonishing views of V838 to date.

More at ESA Website


Posted @ 1:04 PM by kinzi


 

Friday, October 27, 2006

 NASA's Spitzer Peels Back Layers of Star's Explosion 

Astronomers using NASA's infrared Spitzer Space Telescope have discovered that an exploded star, named Cassiopeia A, blew up in a somewhat orderly fashion, retaining much of its original onion-like layering.

Cassiopeia A, or Cas A for short, is what is known as a supernova remnant. The original star, about 15 to 20 times more massive than our sun, died in a cataclysmic "supernova" explosion relatively recently in our own Milky Way galaxy. Like all mature massive stars, the Cas A star was once neat and tidy, consisting of concentric shells made up of various elements. The star's outer skin consisted of lighter elements, such as hydrogen; its middle layers were lined with heavier elements like neon; and its core was stacked with the heaviest elements, such as iron.

Until now, scientists were not exactly sure what happened to the Cas A star when it ripped apart. One possibility is that the star exploded in a more or less uniform fashion, flinging its layers out in successive order. If this were the case, then those layers should be preserved in the expanding debris. Previous observations revealed portions of some of these layers, but there were mysterious gaps.

Spitzer was able to solve the riddle. It turns out that parts of the Cas A star had not been shot out as fast as others when the star exploded. Imagine an onion blasting apart with some layered chunks cracking off and zooming away, and other chunks from a different part of the onion shooting off at slightly slower speeds.

How did Spitzer find the missing puzzle pieces? As the star's layers whiz outward, they are ramming, one by one, into a shock wave from the explosion and heating up. Material that hit the shock wave sooner has had more time to heat up to temperatures that radiate X-ray and visible light. Material that is just now hitting the shock wave is cooler and glowing with infrared light. Consequently, previous X-ray and visible-light observations identified hot, deep-layer material that had been flung out quickly, but not the cooler missing chunks that lagged behind. Spitzer's infrared detectors were able to find the missing chunks – gas and dust consisting of the middle-layer elements neon, oxygen and aluminum.

Cassiopeia A is the ideal target for studying the anatomy of a supernova explosion. Because it is young and relatively close to our solar system, it is undergoing its final death throes right in front of the watchful eyes of various telescopes. In a few hundred years or so, Cas A's scattered remains will have completely mixed together, forever erasing important clues about how the star lived and died.

For more information about Spitzer, visit http://www.nasa.gov/spitzer

or www.spitzer.caltech.edu/spitzer.

JPL Newletter. Released date: October 26, 2006


Posted @ 1:19 PM by kinzi


 

 ESA to Launch a Space Telescope for Finding Earth-like Planets 

The COROT space telescope is proceeding smoothly towards its launch in December 2006. Once in orbit, COROT will become the first spacecraft devoted to the search for rocky planets, similar to our own Earth. COROT will also delve into the centres of hundreds or even thousands of stars.

More at:
ESA website


Posted @ 1:15 PM by kinzi


 

Wednesday, October 18, 2006

 Hubble's View of Colliding Galaxies 

Image Credit: ESA/NASA

A new Hubble image of the Antennae galaxies is the sharpest yet of this
merging pair of galaxies. As the two galaxies smash together, thousand
of millions of stars are born, mostly in groups and clusters of stars. View the larger size here.

Full Story
Image Credit: ESA/NASA


Posted @ 1:39 PM by kinzi


 

Tuesday, October 17, 2006

 Latest Picture from Mars Reconnaissance Orbiter 

Image Credit: NASA

This enhanced-color view shows gullies in an unnamed crater in the Terra Sirenum region of Mars. View the original size here

And all new released images can be accessed here
Image credit: NASA


Posted @ 4:01 PM by kinzi


 

Wednesday, October 11, 2006

 Jupiter's Red Spot Jr. Raging Up 

Image Credit: NASA

According to recent Hubble's observation, Jupiter's little Red Spot is getting stronger, and now it has a wind speed of approximately 400 miles per hour, that almost equals to the wind speed at its sibling, the Great Red Spot. The little Red Spot is actually a giant storm that's about the size of Earth. It was formed from three smaller white-colored storms that merged together and has been observed since 1940s. The effect of storm intensity will eventually change the colour of the storm, according to researcher.

Full Story...


Posted @ 3:26 PM by kinzi


 

Tuesday, October 10, 2006

 Confirmed by Hubble, Epsilon Eridani B is the Closest Exoplanet 

The planet that detected in 2000 and orbiting a Sun-like star is confirmed to co-exist with debris disks around the parent star. The planet orbits its star, Epsilon Eridani, every 6.9 years and has 1.5 times the mass of Jupiter. The star is located 10.5 light years away, that makes this planet to be the closest extrasolar planet to us. Observation from Hubble indicated that this star is young, only 800 million years old that is why it still retains its debris disk.

Epsilon Eridani has long captivated the attention of science fiction writers, as well as astronomers. In 1960, years before the first extrasolar planet was detected, astronomer Frank Drake listened for radio transmissions from inhabitants of any possible planets around Epsilon Eridani as part of Project Ozma's search for intelligent extraterrestrial life. In the fictional "Star Trek" universe, Epsilon Eridani is considered by some fans to be the parent star for the planet Vulcan, Mr. Spock's home.

Full Story...


Posted @ 7:08 PM by kinzi


 

Sunday, October 08, 2006

 New picture from Sharp Vision of Mars Orbiter Released 

Image Credit: NASA

This is the new picture released by NASA from Mars Reconnaissance Orbiter. It shows also here the mars rover 'Opportunity' examining the Victoria crater. A stunning picture!

Visit MRO site for more details.


Posted @ 1:03 PM by kinzi


 

Friday, October 06, 2006

 'Chinese Lantern' Technique Helps Track Clouds at Saturn 

image credit: NASA
A new image of Saturn demonstrates a technique that creates a 'Chinese lantern' effect, showing Saturn's deep clouds silhouetted against the planet's warm, glowing interior. Seen this way, Saturn's interior shows surprising activity underneath the overlying haze, with a great variety of cloud shapes and sizes. Because upper-level hazes and clouds obscure the view of these deep clouds in visible light, imaging clouds in the depths of Saturn is not practical using visible-light cameras. Several recent images obtained by Cassini’s visual and infrared mapping spectrometer were combined in a way that highlights the deep clouds in silhouette against the background radiation of heat generated by Saturn's interior. This literally lights the planet from the inside, like a lantern.

Clouds and hazes in Saturn's northern hemisphere are noticeably thinner than those in its southern hemisphere. This is thought to be a seasonal effect; this idea will be tested as Saturn's northern hemisphere enters springtime in the next few years.
Bright red colors indicate areas relatively free of deep-level clouds and particles, while darker red colors are cloudy regions. Images like these show Saturn's deep clouds under both daytime and nighttime conditions.

JPL Newsletter - Released date October 5


Posted @ 8:59 PM by kinzi


 

Thursday, October 05, 2006

 Hubble Survey Finds Numbers of Extrasolar Planets 

A Hubble Survey called the Sagittarius Window Eclipsing Extrasolar Planet Search (SWEEPS) yielded a finding of Jupiter-sized planets orbiting very close to their parent stars in the central region of our galaxy. The survey covers 180.000 stars. The astronomers used a planet transit technique for the planet findings. Among the those new exoplanets, one has the shortest orbital period, named SWEEPS-10, swings around its star in 10 hours. Located only 740,000 miles from its star, the planet is among the hottest ever detected. It has an estimated temperature of approximately 3,000 degrees Fahrenheit.

More Story


Posted @ 2:40 PM by kinzi


 

 Hubble Eyes Dark Clouds on Uranus 

Hubble spotted dark cloud formation in Uranus atmosphere. Measuring 1,100 miles by 1,900 miles (1,700 kilometers by 3,000 kilometers), the dark cloud is located at a latitude of 27 degrees in Uranus's northern hemisphere, which is just now becoming fully exposed to sunlight after many years of being in shadow. The development of a dark spot may be a signal of the oncoming uranian northern spring, said researchers.

Image Credit: NASA

More Story


Posted @ 2:35 PM by kinzi


 

Sunday, October 01, 2006

 NASA's New Mars Camera Gives Dramatic View of Planet 

Mars is ready for its close-up. The highest-resolution camera ever to orbit Mars is returning low-altitude images to Earth from NASA's Mars Reconnaissance Orbiter.Rocks and surface features as small as armchairs are revealed in the first image from NASA's Mars Reconnaissance Orbiter since the spacecraft maneuvered into its final, low-altitude orbital path. The imaging of the red planet at this resolution heralds a new era in Mars exploration.

The image of a small fraction of Mars' biggest canyon reached Earth on Friday,
the beginning of a week of tests for the High Resolution Imaging Science Experiment
and other instruments on NASA's Mars Reconnaissance Orbiter. "We are elated at the sharpness of the image, revealing such fine detail in the landscape," said Dr. Alfred McEwen of the University of Arizona, Tucson, who is the principal investigator for this camera. The target area includes the deepest part of Ius Chasma, one portion of the vast Valles Marineris canyon. Valles Marineris is the largest known canyon in the solar system, as long as the distance from California to New York.

The image is available online at
http://www.nasa.gov/mission_pages/MRO/multimedia/mro-20060929a.html

and http://hiroc.lpl.arizona.edu/images/TRA/TRA_000823_1720/

The camera returned test images after Mars Reconnaissance Orbiter went into orbit around Mars on March 10, 2006, but those were from altitudes more than eight times as high as the orbiter is flying now. Since March, the spacecraft has shrunk its orbit by dipping more than 400 times into the top of the Martian atmosphere to shave
velocity. It is now flying in its final, nearly circular orbit at altitudes of 250 to 316 kilometers (155 to 196 miles). The orbit will remain this shape and size for the mission's two-year primary science phase, which begins in November.

During its primary science phase, Mars Reconnaissance Orbiter will return more data about the red planet than all previous missions combined, pouring data to Earth at about 10 times the rate of any earlier Mars spacecraft. Scientists will analyze the information to gain a better understanding of the distribution and history of
Mars' water - whether ice, vapor or liquid - and of the processes that formed and modified the planet's surface. In addition to the high-resolution camera, the orbiter's science payload includes a mineral-identifying spectrometer, a ground-penetrating radar, a context camera for imaging wide swaths of the surface, a wide-angle color imager for monitoring the entire planet daily, and an instrument for mapping and monitoring water vapor
and other constituents in the atmosphere.

For most of October, Mars will be passing nearly behind the sun from Earth's perspective. Communication will be intermittent. Activities will be minimal for Mars Reconnaissance Orbiter and other spacecraft at Mars during this time, and they will resume in early November.

JPL Newsletter


Posted @ 9:01 PM by kinzi


 



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    The Oort cloud, is a postulated spherical cloud of comets situated about 50,000 to 100,000 AU from the Sun. This is approximately 1000 times the distance from the Sun to Pluto or roughly one light year, almost a quarter of the distance from the Sun to Proxima Centauri, the star nearest the Sun. The Oort cloud would have its inner disk at the ecliptic from the Kuiper belt. Although no direct observations have been made of such a cloud, it is believed to be the source of most or all comets entering the inner solar system (some short-period comets may come from the Kuiper belt), based on observations of the orbits of comets.
    Source: Wikipedia

     
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