Explanation:
Are asteroids dangerous? Some are, but the likelihood of a dangerous asteroid
striking the Earth during any given year is low. Because some past mass
extinction events have been linked to asteroid impacts, however, humanity has
made it a priority to find and catalog those asteroids that may one day affect
life on Earth. Pictured above are the orbits of the over 1,000 known
Potentially Hazardous Asteroids (PHAs). These documented tumbling boulders of
rock and ice are over 140 meters across and will pass within 7.5 million
kilometers of Earth -- about 20 times the distance to the Moon. Although none
of them will strike the Earth in the next 100 years -- not all PHAs have been
discovered, and past 100 years, many orbits become hard to predict. Were an
asteroid of this size to impact the Earth, it could raise dangerous tsunamis,
for example. Of course rocks and ice bits of much smaller size strike the Earth
every day, usually pose no danger, and sometimes creating memorable fireball
and meteor displays
در تاریخ سیاره ی زمین ، گونه ی انسان دیر ، - بسیار دیر- پدید آمد؛ اما در همین زمان کوتاهی که بر روی زمین بوده است ، " دست آدمی" ، تغییرات ژرفی در هوا، در آب و خاک ، در دیگر موجودات زنده و در همه ی نظامی که بخش های گونه گون آن در پیوند بهم فشرده با یکدیگر ، بر هم کنش دارند و محیط زندگی او را می سازند، پدید آورده است . همه ی این ها در آخرین لحظه ی " زمان زمین شناسی " ، روی داده است .
۱۳۹۲ اسفند ۷, چهارشنبه
Flowing in, Flowing out of Aelia
This
colorful composite image from NASA's Dawn mission shows the flow of material
inside and outside a crater called Aelia on the giant asteroid Vesta. The area
is around 14 degrees south latitude. The images that went into this composite
were obtained by Dawn's framing camera from September to October 2011.
To
the naked eye, these structures would not be seen. But here, they stand out in
blue and red.
The
crater has a diameter of 2.7 miles (4.3 kilometers). The exact origin of the
flow structures is unknown. A possible explanation is that the impact that
produced the crater could have created liquid material with different minerals
than the surroundings.
The
composite image was created by assigning ratios of color information collected
from several color filters in visible light and near-infrared light to maximize
subtle differences in lithology (the physical characteristics of rock units,
such as color, texture and composition). The color scheme pays special attention
to the iron-rich mineral pyroxene.
The
Dawn mission to Vesta and Ceres is managed by NASA's Jet Propulsion Laboratory,
a division of the California Institute of Technology in Pasadena, for NASA's
Science Mission Directorate, Washington. The University of California, Los
Angeles, is responsible for overall Dawn mission science. The Dawn framing
cameras were developed and built under the leadership of the Max Planck
Institute for Solar System Research, Katlenburg-Lindau, Germany, with
significant contributions by DLR German Aerospace Center, Institute of
Planetary Research, Berlin, and in coordination with the Institute of Computer
and Communication Network Engineering, Braunschweig. The framing camera project
is funded by the Max Planck Society, DLR and NASA.
The Pleiades Deep and Dusty
Image Credit & Copyright: David
Lane
Explanation:
The well known Pleiades star cluster is slowly destroying part of a passing
cloud of gas and dust. The Pleiades is the brightest open cluster of stars on
Earth's sky and can be seen from almost any northerly location with the unaided
eye. The passing young dust cloud is thought to be part of Gould's belt, an
unusual ring of young star formation surrounding the Sun in the local Milky Way
Galaxy. Over the past 100,000 years, part of Gould's belt is by chance moving
right through the older Pleiades and is causing a strong reaction between stars
and dust. Pressure from the stars' light significantly repels the dust in the
surrounding blue reflection nebula, with smaller dust particles being repelled
more strongly. A short-term result is that parts of the dust cloud have become
filamentary and stratified, as seen in the above deep-exposure image.
Aurora over New Zealand
Image Credit & Copyright: David
Weir (Earth and Sky Ltd.)
Explanation:
Sometimes the more you look at an image, the more you see. Such may be the case
for this beautiful nighttime panorama taken last week in New Zealand. Visible
right off, on the far left, are common clouds, slightly altered by the digital
fusion of combining 11 separate 20-second exposures. More striking, perhaps, is
the broad pink aurora that dominates the right part of the image, a less common
auroral color that is likely tinted by excited oxygen atoms high in Earth's
atmosphere. Keep looking and you might notice a bright light just beyond the
mountain on the left. That is the rising Moon -- and an even closer look will
reveal faint crepuscular rays emanating from it. Musing over the image center
may cause you to notice the central band of the Milky Way Galaxy which here
appears to divide, almost vertically, the left clouds from the right aurora.
Inspecting the upper right of the image reveals a fuzzy patch, high in the sky,
that is the Small Magellanic Cloud. Numerous stars discretely populate the
distant background. Back on Earth, the image foreground features two domes of
the Mt. John University Observatory and a camera tripod looking to capture much
of this scene over a serene Lake Tekapo.
۱۳۹۲ اسفند ۱, پنجشنبه
Inside the Eagle Nebula
Credit & Copyright: T. A. Rector
& B. A. Wolpa, NOAO, AURA
Explanation:
From afar, the whole thing looks like an Eagle. A closer look at the Eagle
Nebula, however, shows the bright region is actually a window into the center
of a larger dark shell of dust. Through this window, a brightly-lit workshop
appears where a whole open cluster of stars is being formed. In this cavity
tall pillars and round globules of dark dust and cold molecular gas remain
where stars are still forming. Already visible are several young bright blue
stars whose light and winds are burning away and pushing back the remaining
filaments and walls of gas and dust. The Eagle emission nebula, tagged M16,
lies about 6500 light years away, spans about 20 light-years, and is visible
with binoculars toward the constellation of the Serpent (Serpens). This picture
combines three specific emitted colors and was taken with the 0.9-meter
telescope on Kitt Peak, Arizona, USA.
NGC 2359: Thor's Helmet
Image Credit & Copyright: Bob and
Janice Fera (Fera Photography)
Explanation:
This helmet-shaped cosmic cloud with wing-like appendages is popularly called
Thor's Helmet. Heroically sized even for a Norse god, Thor's Helmet is about 30
light-years across. In fact, the helmet is more like an interstellar bubble,
blown as a fast wind from the bright, massive star near the bubble's center
sweeps through a surrounding molecular cloud. Known as a Wolf-Rayet star, the
central star is an extremely hot giant thought to be in a brief, pre-supernova
stage of evolution. Cataloged as NGC 2359, the nebula is located about 15,000
light-years away in the constellation Canis Major. The sharp image, made using
broadband and narrowband filters, captures striking details of the nebula's
filamentary structures. It shows off a blue-green color from strong emission
due to oxygen atoms in the glowing gas.
۱۳۹۲ بهمن ۲۶, شنبه
Hunter's Moon over the Alps
Image Credit & Copyright: Stefano
De Rosa
Explanation:
A Full Moonset can be a dramatic celestial sight, and Full Moons can have many
names. Late October's Full Moon, the second Full Moon after the northern
hemisphere autumnal equinox, has been traditionally called the Hunter's Moon.
According to lore, the name is a fitting one because this Full Moon lights the
night during a time for hunting in preparation for the coming winter months. In
this scene, last week's Hunter's Moon shines with a rich yellow light, setting
as dawn comes to the Italian Alps. Topping out at over 11,000 feet, the snowy
peak known as Rochemelon glows, just catching the first reddened light of the
rising Sun.
Like a Diamond in the Sky
Image Credit & Copyright: Alex
Cherney (Terrastro, TWAN)
Explanation:
A dark Sun hung over Queensland, Australia on Wednesday morning during a much
anticipated total solar eclipse. Storm clouds threatened to spoil the view
along the northern coast, but minutes before totality the clouds parted.
Streaming past the Moon's edge, the last direct rays of sunlight produced a
gorgeous diamond ring effect in this scene from Ellis Beach between Cairns and
Port Douglas. Winking out in a moment, the diamond didn't last forever though.
The area was plunged into darkness for nearly 2 minutes as the Moon's shadow
swept off shore toward Australia's Great Barrier Reef and out into the southern
Pacific. Ranging from 1/4000 to 1/15 seconds long, five separate exposures were
blended in the image to create a presentation similar to the breathtaking
visual experience of the eclipse.
Solar Eclipse over Queensland
Image Credit & Copyright: Phil
Hart
Explanation:
This month's New Moon brought a total solar eclipse to parts of planet Earth on
November 13 (UT). Most of the total eclipse track fell across the southern
Pacific, but the Moon's dark umbral shadow began its journey in northern
Australia on Wednesday morning, local time. From along the track, this
telescopic snapshot captures the Moon's silhouette in skies over Queensland
along the Mulligan highway west of Port Douglas. Almost completely covered, the
Sun's disk is seen still surrounded by a hint of the faint solar corona.
Planet-sized prominences stretch above the active Sun's edge. Sunlight
streaming through gaps in the rugged profile of the lunar limb creates the
brilliant but fleeting Baily's Beads.
Aurora Over White Dome Geyser
Image Credit & Copyright: Robert
Howell
Explanation:
Sometimes both heaven and Earth erupt. Colorful aurorae erupted unexpectedly
earlier this month, with green aurora appearing near the horizon and brilliant
bands of red aurora blooming high overhead. A bright Moon lit the foreground of
this picturesque scene, while familiar stars could be seen far in the distance.
With planning, the careful astrophotographer shot this image mosaic in the
field of White Dome Geyser in Yellowstone National Park in the western USA.
Sure enough, just after midnight, White Dome erupted -- spraying a stream of
water and vapor many meters into the air. Geyser water is heated to steam by
scalding magma several kilometers below, and rises through rock cracks to the
surface. About half of all known geysers occur in Yellowstone National Park.
Although the geomagnetic storm that created these aurorae has since subsided,
eruptions of White Dome Geyser continue about every 30 minutes.
Airglow over Italy
Explanation:
In this serene night skyscape, the Milky Way's graceful arc stretches over
prominent peaks in the Italian Alps known as Tre Cime di Lavaredo. A 180 degree
wide-angle panorama made in four exposures on August 24, the scene does look to
the north and the sky is suffused with an eerie greenish light. Still, the
subtle glowing bands are not aurorae, but airglow. Unlike aurorae powered by
collisions with energetic charged particles and seen at high latitudes, airglow
is due to chemiluminescence, the production of light in a chemical reaction,
and found around the globe. The chemical energy is provided by the Sun's
extreme ultraviolet radiation. Like aurorae, the greenish hue of this airglow
does originate at altitudes of 100 kilometers or so dominated by emission from
excited oxygen atoms. More easily seen near the horizon, airglow keeps the
night sky from ever being completely dark.
On a Blue Moon
Explanation:
Rising at sunset, the gorgeous Full Moon of August 31 became the second Full
Moon in a month. According to modern reckoning, that makes it a Blue Moon. In
fact, parts of the Full Moon do look a little blue in this sharp lunar
portrait. Taken just hours before the exact full phase in delightfully clear
skies over Nottingham, UK, it features eye-catching bright rays extending from
the prominent young crater Tycho in the Moon's southern hemisphere. The
slightly color enhanced image also brings out subtle shades of blue, a real
characteristic of terrain with a high content of titanium oxide and iron. The
blue lunar terrain on the right includes the dark flat expanse of the Sea of
Tranquility and the Apollo 11 landing site.
Light from the Heart
Image Credit & Copyright: César
Blanco González
Explanation:
Sprawling across almost 200 light-years, emission nebula IC 1805 is a mix of
glowing interstellar gas and dark dust clouds about 7,500 light-years away in
the Perseus spiral arm of our galaxy. Stars were born in this region whose
nickname, the Heart Nebula, derives from its Valentine's-Day-appropriate shape.
The clouds themselves are shaped by stellar winds and radiation from massive
hot stars in the nebula's newborn star cluster Melotte 15 about 1.5 million
years young. This deep telescopic image maps the pervasive light of narrow
emission lines from atoms in the nebula to a color palette made popular in
Hubble images of star forming regions. The field of view spans about two
degrees on the sky or four times the diameter of a full moon. The cosmic heart
is found in the constellation of Cassiopeia, the boastful mythical Queen of
Aethiopia .
Downtown Auriga
Image Credit & Copyright: Rogelio
Bernal Andreo (Deep Sky Colors)
Explanation:
Rich in star clusters and nebulae, the ancient constellation of Auriga, the
Charioteer, rides high in northern winter night skies. Spanning nearly 24 full
moons (12 degrees) on the sky, this deep telescopic mosaic view recorded in
January shows off some of Auriga's most popular sights for cosmic tourists. The
crowded field sweeps along the plane of our Milky Way galaxy in the direction
opposite the galactic center. Need directions? Near the bottom of the frame, at
the Charioteer's boundary with Taurus the Bull, the bright bluish star Elnath
is known as both Beta Tauri and Gamma Aurigae. On the far left and almost 300
light-years away, the busy, looping filaments of supernova remnant Simeis 147
cover about 150 light-years. Look toward the right to find emission nebula IC
410, significantly more distant, some 12,000 light-years away. Star forming IC
410 is famous for its embedded young star cluster, NGC 1893, and tadpole-shaped
clouds of dust and gas. The Flaming Star Nebula, IC 405, is just a little
farther along. Its red, convoluted clouds of glowing hydrogen gas are energized
by hot O-type star AE Aurigae. Two of our galaxy's open star clusters, Charles
Messier's M36 and M38 line up in the starfield above, familiar to many
binocular-equipped skygazers.
۱۳۹۲ بهمن ۲۴, پنجشنبه
Supernova remnant in our Milky Way galaxy
This
image shows a composite view of the Crab nebula, an iconic supernova remnant in
our Milky Way galaxy, as viewed by the Herschel Space Observatory and the
Hubble Space Telescope. Herschel is a European Space Agency (ESA) mission with
important NASA contributions, and Hubble is a NASA mission with important ESA
contributions. A wispy and filamentary cloud of gas and dust, the Crab nebula
is the remnant of a supernova explosion that was observed by Chinese
astronomers in the year 1054. The image combines Hubble's view of the nebula at
visible wavelengths, obtained using three different filters sensitive to the
emission from oxygen and sulphur ions and is shown here in blue. Herschel's
far-infrared image reveals the emission from dust in the nebula and is shown
here in red. While studying the dust content of the Crab nebula with Herschel,
a team of astronomers have detected emission lines from argon hydride, a
molecular ion containing the noble gas argon. This is the first detection of a
noble-gas based compound in space. The Herschel image is based on data taken
with the Photoconductor Array Camera and Spectrometer (PACS) instrument at a
wavelength of 70 microns; the Hubble image is based on archival data from the
Wide Field and Planetary Camera 2 (WFPC2). Image credit: ESA/Herschel/PACS/MESS
Key Programme Supernova Remnant Team;
NASA, ESA and Allison Loll/Jeff Hester (Arizona State University)
Artist's Concept of Europa Water Vapor Plume
This
is an artist's concept of a plume of water vapor thought to be ejected off the
frigid, icy surface of the Jovian moon Europa, located about 500 million miles
(800 million kilometers) from the sun. Spectroscopic measurements from NASA's
Hubble Space Telescope led scientists to calculate that the plume rises to an
altitude of 125 miles (201 kilometers) and then it probably rains frost back
onto the moon's surface. Previous findings already pointed to a subsurface
ocean under Europa's icy crust.
The
Hubble Space Telescope is a project of international cooperation between NASA
and the European Space Agency. NASA's Goddard Space Flight Center manages the
telescope. The Space Telescope Science Institute (STScI) conducts Hubble
science operations. STScI is operated for NASA by the Association of
Universities for Research in Astronomy, Inc., in Washington, D.C.
To
view the images of the evidence for plumes visit:
http://www.nasa.gov/content/goddard/hubble-europa-water-vapor. For more
information about the Hubble Space Telescope, visit: http://www.nasa.gov/hubble.
Moon Meets Morning Star
Image Credit & Copyright: Kwon, O
Chul (TWAN)
Explanation:
Rising in the dark hours before dawn, wandering Venus now shines as the
brilliant morning star. Its close conjunction with the Moon on August 13 was
appreciated around planet Earth. But skygazers in eastern Asia were also
treated to a lunar occultation, the waning crescent Moon passing directly in
front of the bright planet in still dark skies. This composite image
constructed from frames made at 10 minute intervals follows the celestial
performance (vimeo video) from above the city lights and clouds over Taebaek,
Korea. The occultation begins near the horizon and progresses as the pair
rises. Venus first disappears behind the Moon's sunlit crescent, emerging
before dawn from the dark lunar limb.
A Particle Beam Jet forms HH 24
Image Credit: Hubble Legacy Archive,
NASA, ESA - Processing: Judy Schmidt
Explanation:
If you visit HH 24, don't go near the particle beam jet. This potential future
travel advisory might be issued because the powerful jet likely contains
electrons and protons moving hundreds of kilometers per second. The above image
was taken by the Hubble Space Telescope in infrared light in order to better
understand turbulent star forming regions known as Young Stellar Objects
(YSOs). Frequently when a star forms, a disk of dust and gas circles the YSO
causing a powerful central jets to appear. In this case, the energetic jets are
creating, at each end, Herbig-Haro object 24 (HH 24), as they slam into the
surrounding interstellar gas. The entire star forming region lies about 1,500
light years distant in the Orion B molecular cloud complex. Due to their
rarity, jets like that forming HH 24 are estimated to last only a few thousand
years.
The Beautiful Trifid
Image Credit & Copyright: Máximo
Ruiz
Explanation:
The beautiful Trifid Nebula is a cosmic study in contrasts. Also known as M20,
it lies about 5,000 light-years away toward the nebula rich constellation
Sagittarius. A star forming region in the plane of our galaxy, the Trifid
illustrates three different types of astronomical nebulae; red emission nebulae
dominated by light emitted by hydrogen atoms, blue reflection nebulae produced
by dust reflecting starlight, and dark nebulae where dense dust clouds appear
in silhouette. The bright red emission region, roughly separated into three
parts by obscuring dust lanes, lends the Trifid its popular name. But in this
sharp, colorful scene, the red emission is also surrounded by the the telltale
blue haze of reflection nebulae. Pillars and jets sculpted by newborn stars,
below and left of the emission nebula's center, appear in Hubble Space
Telescope close-up images of the region. The Trifid Nebula is about 40
light-years across.
Sunspot at Sunset
Image Credit & Copyright: Jo
Hunter
Explanation:
Reddened rays of the setting Sun flooded the skies over Cedar Creek Lake,
southeast of Dallas, Texas, planet Earth on July 6th. And while sunsets may be
the most watched celestial event, this one even offered something extra. A
sunspot so large it was visible to the naked eye is captured in the serene
sunset view, near the center of a solar disk dimmed and distorted by Earth's
dense atomosphere. Telescopic views revealed the spot to be a complex of large
solar active regions composed of sunspots, some larger than planet Earth itself.
The Terraced Night
Image Credit & Copyright: Cui
Yongjiang
Explanation:
Long after sunset on January 25 an unusually intense red airglow floods this
south-looking skyscape. The scene was recorded with a long exposure using a
digital camera over Yunnan Province in southwest China. At best faintly visible
to the eye, the lingering airglow is due to chemiluminescence, the production
of light through chemical excitation. Originating at an altitude similar to
aurora, it can found around the globe. The chemical energy is initially
provided by the Sun's extreme ultraviolet radiation On this night, despite the
luminous atmosphere, the band of the Milky Way clearly stretches above the
horizon with bright star Sirius near the top of the frame. Both airglow and
starry sky are beautifully reflected in region's watery Yuanyang rice terraces
below.
Night Hides the World
Image Credit & Copyright: Babak
Tafreshi (TWAN)
Explanation:
Stars come out as evening twilight fades in this serene skyscape following the
Persian proverb "Night hides the world, but reveals a universe." In
the scene from last November, the Sun is setting over northern Kenya and the
night will soon hide the shores of Lake Turkana, home to many Nile crocodiles.
That region is also known as the cradle of humankind for its abundance of
hominid fossils. A brilliant Venus, then the world's evening star, dominates
the starry night above. But also revealed are faint stars, cosmic dust clouds,
and glowing nebulae along the graceful arc of our own Milky Way galaxy.
NGC 5101 and Friends
Image Credit & Copyright: Martin
Pugh
Explanation:
This sharp telescopic field of view holds two bright galaxies. Barred spiral
NGC 5101 (top right) and nearly edge-on system NGC 5078 are separated on the
sky by about 0.5 degrees or about the apparent width of a full moon. Found
within the boundaries of the serpentine constellation Hydra, both are estimated
to be around 90 million light-years away and similar in size to our own large
Milky Way galaxy. In fact, if they both lie at the same distance their
projected separation would be only 800,000 light-years or so. That's easily
less than half the distance between the Milky Way and the Andromeda Galaxy. NGC
5078 is interacting with a smaller companion galaxy, cataloged as IC 879, seen
just below and left of the larger galaxy's bright core. Even more distant
background galaxies are scattered around the colorful field. Some are even
visible right through the face-on disk of NGC 5101. But the prominent spiky
stars are in the foreground, well within our own Milky Way.
The Heart and Soul Nebulas
Image Credit & Copyright: Leonardo
Orazi
Explanation:
Is the heart and soul of our Galaxy located in Cassiopeia? Possibly not, but
that is where two bright emission nebulas nicknamed Heart and Soul can be
found. The Heart Nebula, officially dubbed IC 1805 and visible in the above
zoomable view on the right, has a shape reminiscent of a classical heart
symbol. Both nebulas shine brightly in the red light of energized hydrogen.
Several young open clusters of stars populate the image and are visible above
in blue, including the nebula centers. Light takes about 6,000 years to reach
us from these nebulas, which together span roughly 300 light years. Studies of
stars and clusters like those found in the Heart and Soul Nebulas have focussed
on how massive stars form and how they affect their environment
Rocket, Meteor, and Milky Way over Thailand
Image Credit & Copyright: Matipon
Tangmatitham
Explanation:
Can the night sky appear both serene and surreal? Perhaps classifiable as
serene in the above panoramic image taken last Friday are the faint lights of
small towns glowing across a dark foreground landscape of Doi Inthanon National
Park in Thailand, as well as the numerous stars glowing across a dark
background starscape. Also visible are the planet Venus and a band of zodiacal
light on the image left. Unusual events are also captured, however. First, the
central band of our Milky Way Galaxy, while usually a common site, appears here
to hover surreally above the ground. Next, a fortuitous streak of a meteor was
captured on the image right. Perhaps the most unusual component is the bright
spot just to the left of the meteor. That spot is the plume of a rising Ariane
5 rocket, launched a few minutes before from Kourou, French Guiana. How lucky
was the astrophotographer to capture the rocket launch in his image? Not lucky
at all -- the image was timed to capture the rocket. What was lucky was how photogenic
-- and perhaps surreal -- the rest of the sky turned out to be.
Clouds, Birds, Moon, Venus
Clouds, Birds, Moon, Venus
Image Credit & Copyright: Isaac
Gutiérrez Pascual (Spain)
Explanation:
Sometimes the sky above can become quite a show. In early September of 2010,
for example, the Moon and Venus converged, creating quite a sight by itself for
sky enthusiasts around the globe. From
some locations, though, the sky was even more picturesque. In the above image
taken in Spain, a crescent Moon and the planet Venus, on the far right, were
captured during sunset posing against a deep blue sky. In the foreground, dark storm clouds loom
across the image bottom, while a white anvil cloud shape appears above. Black
specks dot the frame, caused by a flock of birds taking flight. Very soon after
this picture was taken, however, the birds passed by, the storm ended, and
Venus and the Moon set. Bright Venus
again becomes visible just after sunset this 2013 May and will appear near
Jupiter toward the end of the month.
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