Saturday, 30 August 2014

Caterpillar Comet Poses for Pictures En Route to Mars

by Bob King on August 30, 2014

Comet C/2013 A1 Siding Spring passed between the Small Magellanic Cloud (left) and the rich globular cluster NGC 130 on August 29, 2014. Credit: Rolando Ligustri
Comet C/2013 A1 Siding Spring wriggles between the globular clusters NGC 362 (upper left) and 47 Tucanae (NGC 104) while skirting the edge of the Small Magellanic Cloud on August 29, 2014. Credit: Rolando Ligustri
Now that’s pure gorgeous. As Comet C/2013 A1 Siding Spring sidles towards its October 19th encounter with Mars, it’s passing a trio of sumptuous deep sky objects near the south celestial pole this week. Astrophotographers weren’t going to let the comet’s picturesque alignments pass without notice. Rolando Ligustri captured this remarkable view using a remote, computer-controlled telescope on August 29th. It shows the rich assemblage of stars and star clusters that comprise the Small Magellanic Cloud, one of the Milky Way’s satellite galaxies located 200,000 light years away.

A photo taken one day earlier on August 28th captures the comet and NGC 362 in a tight pairing. Credit: Damian Peach
A photo taken one day earlier on August 28th captures the comet and NGC 362 in close embrace. Credit: Damian Peach
Looking like a fuzzy caterpillar, Siding Spring seems to crawl between the little globular cluster NGC 362 and the  rich swarm called  47 Tucanae, one of the few globulars bright enough to see with the naked eye. C/2013 A1 is currently circumpolar from many locations south of the equator and visible all night long. Glowing at around magnitude +9.5 with a small coma and brighter nucleus, a 6-inch or larger telescope will coax it from a dark sky. Siding Spring dips farthest south on September 2-3 (Dec. -74º) and then zooms northward for Scorpius and Sagittarius. It will encounter additional deep sky objects along the way, most notably the bright open cluster M7 on October 5-6, before passing some 82,000 miles from Mars on October 19th.
Map showing Comet Siding Spring's recent and upcoming travels near the Small Magellanic Cloud. Positions are shown nightly for Alice Springs, Australia. Source: Chris Marriott's SkyMap
Map showing Comet Siding Spring’s recent and upcoming travels near the Small Magellanic Cloud. Positions are shown nightly for Alice Springs, Australia. Source: Chris Marriott’s SkyMap
While the chance of a Mars impact is near zero, the fluffy comet’s fluffy coma and broad tail, both replete with tiny but fast-moving (~125,000 mph) dust particles, might pose a hazard for spacecraft orbiting the Red Planet. Assuming either coma or tail grows broad enough to sweep across the Martian atmosphere, impacting dust might create a spectacular meteor shower. Mars Rover cameras may be used to photograph the comet before the flyby and to capture meteors during its closest approach. NASA plans to ‘hide’ its orbiting probes on the opposite side of the planet for a brief time during the approximately 4-hour-long encounter just in case.
Today, Siding Spring’s coma or temporary atmosphere measures about 12,000 miles (19,300 km) wide. While I can’t get my hands on current dust production rates, in late January, when it was farther from the sun than at present, C/2013 A1 kicked out ~800,000 lbs per hour (~100 kg/sec). On October 19th, observers across much of the globe with 6-inch or larger instruments will witness the historic encounter with their own eyes at dusk in the constellation Sagittarius.

Friday, 29 August 2014

US Heavy Lift Mars Rocket Passes Key Review and NASA Sets 2018 Maiden Launch Date

by Ken Kremer on August 28, 2014

Artist concept of NASA’s Space Launch System (SLS) 70-metric-ton configuration launching to space. SLS will be the most powerful rocket ever built for deep space missions, including to an asteroid and ultimately to Mars. Credit: NASA/MSFC
Artist concept of NASA’s Space Launch System (SLS) 70-metric-ton configuration launching to space. SLS will be the most powerful rocket ever built for deep space missions, including to an asteroid and ultimately to Mars. Credit: NASA/MSFC
Story updated
After a thorough review of cost and engineering issues, NASA managers formally approved the development of the agency’s mammoth heavy lift rocket – the Space Launch System or SLS – which will be the world’s most powerful rocket ever built and is intended to take astronauts farther beyond Earth into deep space than ever before possible – to Asteroids and Mars.
The maiden test launch of the SLS is targeted for November 2018 and will be configured in its initial 70-metric-ton (77-ton) version, top NASA officials announced at a briefing for reporters on Aug. 27.
On its first flight known as EM-1, the SLS will also loft an uncrewed Orion spacecraft on an approximately three week long test flight taking it beyond the Moon to a distant retrograde orbit, said William Gerstenmaier, associate administrator for the Human Explorations and Operations Mission Directorate at NASA Headquarters in Washington, at the briefing.
Previously NASA had been targeting Dec. 2017 for the inaugural launch from the Kennedy Space Center in Florida – a slip of nearly one year.
But the new Nov. 2018 target date is what resulted from the rigorous assessment of the technical, cost and scheduling issues.
This artist concept shows NASA’s Space Launch System, or SLS, rolling to a launch pad at Kennedy Space Center at night. SLS will be the most powerful rocket in history, and the flexible, evolvable design of this advanced, heavy-lift launch vehicle will meet a variety of crew and cargo mission needs.   Credit:  NASA/MSFC
This artist concept shows NASA’s Space Launch System, or SLS, rolling to a launch pad at Kennedy Space Center at night. SLS will be the most powerful rocket in history, and the flexible, evolvable design of this advanced, heavy-lift launch vehicle will meet a variety of crew and cargo mission needs. Credit: NASA/MSFC
The decision to move forward with the SLS comes after a wide ranging review of the technical risks, costs, schedules and timing known as Key Decision Point C (KDP-C), said Associate Administrator Robert Lightfoot, at the briefing. Lightfoot oversaw the review process.
“After rigorous review, we’re committing today to a funding level and readiness date that will keep us on track to sending humans to Mars in the 2030s – and we’re going to stand behind that commitment,” said Lightfoot. “Our nation is embarked on an ambitious space exploration program.”
“We are making excellent progress on SLS designed for missions beyond low Earth orbit,” Lightfoot said. “We owe it to the American taxpayers to get it right.”
He said that the development cost baseline for the 70-metric ton version of the SLS was $7.021 billion starting from February 2014 and continuing through the first launch set for no later than November 2018.
Lightfoot emphasized that NASA is also building an evolvable family of vehicles that will increase the lift to an unprecedented lift capability of 130 metric tons (143 tons), which will eventually enable the deep space human missions farther out than ever before into our solar system, leading one day to Mars.
“It’s also important to remember that we’re building a series of launch vehicles here, not just one,” Lightfoot said.
Blastoff of NASA’s Space Launch System (SLS) rocket and Orion crew vehicle from the Kennedy Space Center, Florida.   Credit: NASA/MSFC
Blastoff of NASA’s Space Launch System (SLS) rocket and Orion crew vehicle from the Kennedy Space Center, Florida. Credit: NASA/MSFC
Lightfoot and Gerstenmaier both indicated that NASA hopes to launch sooner, perhaps by early 2018.
“We will keep the teams working toward a more ambitious readiness date, but will be ready no later than November 2018,” said Lightfoot.
The next step is conduct the same type of formal KDP-C reviews for the Orion crew vehicle and Ground Systems Development and Operations programs.
The first piece of SLS flight hardware already built and to be tested in flight is the stage adapter that will fly on the maiden launch of Orion this December atop a ULA Delta IV Heavy booster during the EFT-1 mission.
The initial 70-metric-ton (77-ton) version of the SLS stands 322 feet tall and provides 8.4 million pounds of thrust. That’s already 10 percent more thrust at launch than the Saturn V rocket that launched NASA’s Apollo moon landing missions, including Apollo 11, and it can carry more than three times the payload of the now retired space shuttle orbiters.
The core stage towers over 212 feet (64.6 meters) tall with a diameter of 27.6 feet (8.4 m) and stores cryogenic liquid hydrogen and liquid oxygen. Boeing is the prime contractor for the SLS core stage.
The first stage propulsion is powered by four RS-25 space shuttle main engines and a pair of enhanced five segment solid rocket boosters (SRBs) also derived from the shuttles four segment boosters.
The pressure vessels for the Orion crew capsule, including EM-1 and EFT-1, are also being manufactured at MAF. And all of the External Tanks for the space shuttles were also fabricated at MAF.
The airframe structure for the first Dream Chaser astronaut taxi to low Earth orbit is likewise under construction at MAF as part of NASA’s commercial crew program.
The first crewed flight of the SLS is set for the second launch on the EM-2 mission around the 2020/2021 time frame, which may visit a captured near Earth asteroid.
Stay tuned here for Ken’s continuing Earth and Planetary science and human spaceflight news.

Wednesday, 27 August 2014

Boeing unveiled full scale mockup of their commercial  CST-100  'Space Taxi' on June 9, 2014 at its intended manufacturing facility at the Kennedy Space Center in Florida.  The private vehicle will launch US astronauts to low Earth orbit and the ISS from US soil.   Credit: Ken Kremer - kenkremer.com
Boeing unveiled full scale mockup of their commercial CST-100 ‘Space Taxi’ on June 9, 2014 at its intended manufacturing facility at the Kennedy Space Center in Florida. The private vehicle will launch US astronauts to low Earth orbit and the ISS from US soil. Credit: Ken Kremer – kenkremer.com
In the ‘new race to space’ to restore our capability to launch Americans to orbit from American soil with an American-built commercial ‘space taxi’ as rapidly and efficiently as possible, Boeing has moved to the front of the pack with their CST-100 spaceship by completing all their assigned NASA milestones on time and on budget in the current phase of the agency’s Commercial Crew Program (CCP).

Monday, 25 August 2014

Get this great Celestron 6" SC XLT right here at astronomyandtelescopesforyou.com

Saturday, 23 August 2014

New mass map of a distant galaxy cluster is the most precise yet

Stunning new observations from Frontier Fields

24 July 2014
Astronomers using the NASA/ESA Hubble Space Telescope have mapped the mass within a galaxy cluster more precisely than ever before. Created using observations from Hubble's Frontier Fields observing programme, the map shows the amount and distribution of mass within MCS J0416.1–2403, a massive galaxy cluster found to be 160 trillion times the mass of the Sun. The detail in this mass map was made possible thanks to the unprecedented depth of data provided by new Hubble observations, and the cosmic phenomenon known as strong gravitational lensing.
Measuring the amount and distribution of mass within distant objects in the Universe can be very difficult. A trick often used by astronomers is to explore the contents of large clusters of galaxies by studying the gravitational effects they have on the light from very distant objects beyond them. This is one of the main goals of Hubble's Frontier Fields, an ambitious observing programme scanning six different galaxy clusters — including MCS J0416.1–2403, the cluster shown in this stunning new image [1].
Large clumps of mass in the Universe warp and distort the space-time around them. Acting like lenses, they appear to magnify and bend light that travels through them from more distant objects [2].
Despite their large masses, the effect of galaxy clusters on their surroundings is usually quite minimal. For the most part they cause what is known as weak lensing, making even more distant sources appear as only slightly more elliptical or smeared across the sky. However, when the cluster is large and dense enough and the alignment of cluster and distant object is just right, the effects can be more dramatic. The images of normal galaxies can be transformed into rings and sweeping arcs of light, even appearing several times within the same image. This effect is known as strong lensing, and it is this phenomenon, seen around the six galaxy clusters targeted by the Frontier Fields programme, that has been used to map the mass distribution of MCS J0416.1–2403, using the new Hubble data.
"The depth of the data lets us see very faint objects and has allowed us to identify more strongly lensed galaxies than ever before," explains Mathilde Jauzac of Durham University, UK, and Astrophysics & Cosmology Research Unit, South Africa, lead author of the new Frontier Fields paper. "Even though strong lensing magnifies the background galaxies they are still very far away and very faint. The depth of these data means that we can identify incredibly distant background galaxies. We now know of more than four times as many strongly lensed galaxies in the cluster than we did before."
Using Hubble's Advanced Camera for Surveys, the astronomers identified 51 new multiply imaged galaxies around the cluster, quadrupling the number found in previous surveys and bringing the grand total of lensed galaxies to 68. Because these galaxies are seen several times this equates to almost 200 individual strongly lensed images which can be seen across the frame. This effect has allowed Jauzac and her colleagues to calculate the distribution of visible and dark matter in the cluster and produce a highly constrained map of its mass [3].
"Although we’ve known how to map the mass of a cluster using strong lensing for more than twenty years, it’s taken a long time to get telescopes that can make sufficiently deep and sharp observations, and for our models to become sophisticated enough for us to map, in such unprecedented detail, a system as complicated as MCS J0416.1–2403," says team member Jean-Paul Kneib.
By studying 57 of the most reliably and clearly lensed galaxies, the astronomers modelled the mass of both normal and dark matter within MCS J0416.1-2403. "Our map is twice as good as any previous models of this cluster!" adds Jauzac.
The total mass within MCS J0416.1-2403 — modelled to be over 650 000 light-years across — was found to be 160 trillion times the mass of the Sun. This measurement is several times more precise than any other cluster map, and is the most precise ever produced [4]. By precisely pinpointing where the mass resides within clusters like this one, the astronomers are also measuring the warping of space-time with high precision.
"Frontier Fields' observations and gravitational lensing techniques have opened up a way to very precisely characterise distant objects — in this case a cluster so far away that its light has taken four and a half billion years to reach us," adds Jean-Paul Kneib. "But, we will not stop here. To get a full picture of the mass we need to include weak lensing measurements too. Whilst it can only give a rough estimate of the inner core mass of a cluster, weak lensing provides valuable information about the mass surrounding the cluster core."
The team will continue to study the cluster using ultra-deep Hubble imaging and detailed strong and weak lensing information to map the outer regions of the cluster as well as its inner core, and will thus be able to detect substructures in the cluster's surroundings. They will also take advantage of X-ray measurements of hot gas and spectroscopic redshifts to map the contents of the cluster, evaluating the respective contribution of dark matter, gas and stars [5].
Combining these sources of data will further enhance the detail of this mass distribution map, showing it in 3D and including the relative velocities of the galaxies within it. This paves the way to understanding the history and evolution of this galaxy cluster.
The results of the study will be published online in Monthly Notices of the Royal Astronomical Society on 24 July 2014.









Using data gathered by NASA's Lunar Reconnaissance Orbiter (LRO) mission, scientists believe they have solved a mystery from one of the solar system's coldest regions -- a permanently shadowed crater on the moon. They have explained how energetic particles penetrating lunar soil can create molecular hydrogen from water ice. The finding provides insight into how radiation can change the chemistry of water ice throughout the solar system.
Space scientists from the University of New Hampshire and NASA's Goddard Space Flight Center have published their results online in the Journal of Geophysical Research (JGR): Planets. Lead author of the paper is research scientist Andrew Jordan of the University of New Hampshire's Institute for the Study of Earth, Oceans, and Space (EOS).
Discovering molecular hydrogen on the moon was a surprise result from NASA's Lunar Crater Observation Sensing Satellite (LCROSS) mission, which crash-landed the LCROSS satellite's spent Centaur rocket at 5,600 miles per hour into the Cabeus crater in the permanently shadowed region of the moon. These regions have never been exposed to sunlight and have remained at temperatures near absolute zero for billions of years, thus preserving the pristine nature of the lunar soil, or regolith.
Instruments on board LCROSS trained on the resulting immense debris plume detected water vapor and water ice, the mission's hoped-for quarry, while LRO, already in orbit around the moon, saw molecular hydrogen -- a surprise.
"LRO's Lyman Alpha Mapping Project, or LAMP, detected the signature of molecular hydrogen, which was unexpected and unexplained," says Jordan.
Jordan's JGR paper, "The formation of molecular hydrogen from water ice in the lunar regolith by energetic charged particles," quantifies an explanation of how molecular hydrogen, which is composed of two hydrogen atoms and denoted chemically as H2, may be created below the moon's surface.
"After the finding, there were a couple of ideas for how molecular hydrogen could be formed but none of them seemed to work for the conditions in the crater or with the rocket impact." Jordan says. "Our analysis shows that the galactic cosmic rays, which are charged particles energetic enough to penetrate below the lunar surface, can dissociate the water, H2O, into H2 through various potential pathways."
That analysis was based on data gathered by the Cosmic Ray Telescope for the Effects of Radiation (CRaTER) instrument aboard the LRO spacecraft. Jordan is a member of the CRaTER scientific team, which is headed up by principal investigator Nathan Schwadron of EOS. Schwadron, a co-author on the JGR paper, was the first to suggest energetic particles as the possible mechanism for creating molecular hydrogen.
CRaTER characterizes the global lunar radiation environment by measuring radiation dose rates from galactic cosmic rays and solar energetic particles. Says Jordan, "We used the CRaTER measurements to get a handle on how much molecular hydrogen has been formed from the water ice via charged particles." Jordan's computer model incorporated the CRaTER data and showed that these energetic particles can form between 10 and 100 percent of the H2 measured by LAMP.
The study notes that narrowing down that percent range requires particle accelerator experiments on water ice to more accurately gauge the number of chemical reactions that result per unit of energy deposited by cosmic rays and solar energetic particles.




Wednesday, 20 August 2014

Australian Amateur Terry Lovejoy Discovers New Comet

by Bob King on August 19, 2014

The small fuzzy potential comet is at center in this photo taken discovered by Terry Lovejoy. Credit: copyright Alain Maury and Joaquin Fabrega
The fuzzy object at center is new comet C/2014 Q2 (Lovejoy) discovered by Australian amateur astronomer Terry Lovejoy. Copyright Alain Maury and Joaquin Fabrega
It’s confirmed! Australian amateur astronomer Terry Lovejoy just discovered his fifth comet, C/2014 Q2 (Lovejoy). He found it August 17th using a Celestron C8 fitted with a CCD camera at his roll-off roof observatory in Brisbane, Australia. 
Image triplet taken by Terry Lovejoy on which he discovered the comet. The comet moves slightly counterclockwise around the larger fuzzy spot. Credit: Terry Lovejoy
Image triplet taken by Terry Lovejoy of his comet discovery. The comet moves slightly counterclockwise around the larger fuzzy spot over the time frame. Credit: Terry Lovejoy
“I take large sets of image triplets, i.e 3 images per star field and use software to find moving objects,” said Lovejoy.  “The software I use outputs suspects that I check manually by eye.”
Most of what pops up on the camera are asteroids, known comets, or false alarms but not this time. Lovejoy’s latest find is a faint, fuzzy object in the constellation Puppis in the morning sky.
Sky as seen from central South America showing the approximate location of the new comet on August 19 in Puppis near the bright star Canopus. Stellarium
Sky as seen from central South America showing the approximate location of the new comet  (purple circle) on August 19 in Puppis near the bright star Canopus. The view shows the sky facing southeast just before the start of dawn. Stellarium
Glowing a dim magnitude +15, the new comet will be a southern sky object until later this fall when it swings quickly northward soon around the time of perihelion or closest approach to the sun. Lovejoy’s find needs more observations to better refine its orbit, but based on preliminary data, Maik Meyer, founder of the Comets Mailing List, calculates a January 2, 2015 perihelion.
Another photo of C/2014 Q2 taken on August 19, 2014. Credit: Jean-François and Alain Maury
Another photo of C/2014 Q2 taken on August 19, 2014. Credit: Jean-François and Alain Maury
On that date, it will be a healthy 84 million miles from the sun, but one month earlier on December 7, the comet could pass just 6.5 million miles from Earth and be well placed for viewing in amateur telescopes.
Everything’s still a little up in the air right now, so these times and distances are likely to change as fresh observations pour in. Take all predictions with a major grain of salt for the moment.
photographed by NASA astronaut Dan Burbank, Expedition 30 commander, onboard the International Space Station on Dec. 22, 2011. Credit: NASA
Comet Lovejoy (C/2011 W3) photographed by NASA astronaut Dan Burbank, onboard the International Space Station on Dec. 22, 2011 from 250 miles up. Credit: NASA
You might remember some of Terry’s earlier comets. Comet Lovejoy (C/2011 W3), a Kreutz sungrazer discovered in November 2011, passed just 87,000 miles above the sun’s surface. Many astronomers thought it wouldn’t  survive the sun’s heat, yet amazingly, although much of its nucleus burned off, enough material survived to produce a spectacular tail.
Terry Lovejoy
Terry Lovejoy
More recently, Comet Lovejoy (C/2013 R1) thrilled observers as it climbed to naked eye brightness last November, managing to do the impossible at the time and draw our eyes away from Comet ISON.
Congratulations Terry on your new find! May it wax brightly this fall.
* Update: The latest orbit calculation from the Minor Planet Center based on 24 observations now puts perihelion at 164.6 million miles (265 million km) on February 14, 2015. Closest approach to Earth of 93.2 million miles (150 million km) will occur in January.

Monday, 18 August 2014

How many
Earths?

Looking up at the night sky, it's hard not to wonder how many other planets might be circling those pinpricks of light – and how many are home to beings gazing back at us.
Today, we are starting to get a handle on the number of roughly Earth-sized exoplanets that might be suitable for life.

How to spot a planet

We can take a good guess at the number of alien Earths thanks to NASA's Kepler space telescope.
When a planet passes in front of its parent star, it blocks some of the star's light. The Kepler telescope looked for distant worlds by measuring this dip in stars' glow.

signal

In

In the frame

Kepler focused its gaze on the area of sky marked out by this grid of squares near the constellation Cygnus.
The telescope's detectors were trained on some 150,000 target stars in this grid for nearly four years until the end of its active planet-hunting days in May 2013.

In the frame

Kepler focused its gaze on the area of sky marked out by this grid of squares near the constellation Cygnus.
The telescope's detectors were trained on some 150,000 target stars in this grid for nearly four years until the end of its active planet-hunting days in May 2013.
▼ Next▲ Previous

Kepler's haul

The green dots show the possible planets discovered in Kepler's data so far.
To pursue our quest, we must exclude planets that are nothing like our home world. First, let's remove everything twice the diameter of Earth or larger, which are likely to be gas giants like Jupiter and Saturn.
▼ Next▲ Previous

In the Goldilocks zone?

The remaining planets are the right size, but not all of them will be ripe for life, with life-sustaining liquid water.
We can't determine a planet's composition from Kepler's data, but we can see whether a planet seems to orbit in the habitable zone around its parent star.

habitable_zone ▼ Next▲ Previous

These might be like home

This is our best estimate for the number of potentially life-bearing worlds among the planets spotted by Kepler. But we're missing much of the picture.
Kepler could spot only planets that passed between their parent stars and the telescope's viewpoint – even a slight tilt in a planet's orbit could make it invisible to the telescope. And the farther out a planet orbits, the more likely it was to be missed.
tilt ▼ Next▲ Previous

Earths galore

After extrapolating for all the missing worlds, Kepler's field of view becomes dense with planets that may be like Earth.
Now consider this: Kepler observed just 0.28 per cent of the sky. And the telescope was able to peer out to only 3000 light years away, studying less than 5 per cent of the stars in its field of view. So how many Earths might really be out there?
▼ Next▲ Previous

A crowded galaxy

Expanding our view from Kepler's corner of the galaxy to show more of the Milky Way, the sky fills with billions of potentially life-bearing worlds. If we showed them all, the sky would be a mass of green. So now the green dots illustrate stars that might host such planets, visible with a good pair of binoculars on a dark night here on Earth.
From this perspective, the chances that we're alone in the cosmos seem very slim, indeed.
▼ Next▲ Previous

The search continues

The Kepler telescope may no longer be hunting for alien Earths, but more discoveries are sure to come as researchers work through the backlog of data it gathered. In 2017, the search will be taken up by the Transiting Exoplanet Survey Satellite, which will survey nearby stars across the entire sky.
▼ Next▲ Previous

Credits

Thanks to Natalie Batalha, Jon Jenkins and other members of the Kepler mission team for technical advice.
Learn more about the data used in this graphic.
Produced by Adam Becker, MacGregor Campbell and Peter Aldhous.
Published 25 September 2013.
⇧ Back to top ▲ Previous

the frame

Kepler focused its gaze on the area of sky marked out by this grid of squares near the constellation Cygnus.
The telescope's detectors were trained on some 150,000 target stars in this grid for nearly four years until the end of its active planet-hunting days in May 2013.
▼ Next▲ Previous

Kepler's haul

The green dots show the possible planets discovered in Kepler's data so far.
To pursue our quest, we must exclude planets that are nothing like our home world. First, let's remove everything twice the diameter of Earth or larger, which are likely to be gas giants like Jupiter and Saturn.
▼ Next▲ Previous

In the Goldilocks zone?

The remaining planets are the right size, but not all of them will be ripe for life, with life-sustaining liquid water.
We can't determine a planet's composition from Kepler's data, but we can see whether a planet seems to orbit in the habitable zone around its parent star.

habitable_zone ▼ Next▲ Previous

These might be like home

This is our best estimate for the number of potentially life-bearing worlds among the planets spotted by Kepler. But we're missing much of the picture.
Kepler could spot only planets that passed between their parent stars and the telescope's viewpoint – even a slight tilt in a planet's orbit could make it invisible to the telescope. And the farther out a planet orbits, the more likely it was to be missed.
tilt ▼ Next▲ Previous

Earths galore

After extrapolating for all the missing worlds, Kepler's field of view becomes dense with planets that may be like Earth.
Now consider this: Kepler observed just 0.28 per cent of the sky. And the telescope was able to peer out to only 3000 light years away, studying less than 5 per cent of the stars in its field of view. So how many Earths might really be out there?
▼ Next▲ Previous

A crowded galaxy

Expanding our view from Kepler's corner of the galaxy to show more of the Milky Way, the sky fills with billions of potentially life-bearing worlds. If we showed them all, the sky would be a mass of green. So now the green dots illustrate stars that might host such planets, visible with a good pair of binoculars on a dark night here on Earth.
From this perspective, the chances that we're alone in the cosmos seem very slim, indeed.
▼ Next▲ Previous

The search continues

The Kepler telescope may no longer be hunting for alien Earths, but more discoveries are sure to come as researchers work through the backlog of data it gathered. In 2017, the search will be taken up by the Transiting Exoplanet Survey Satellite, which will survey nearby stars across the entire sky.
▼ Next▲ Previous

Credits

Thanks to Natalie Batalha, Jon Jenkins and other members of the Kepler mission team for technical advice.
Learn more about the data used in this graphic.
Produced by Adam Becker, MacGregor Campbell and Peter Aldhous.
Published 25 September 2013.
⇧ Back to top ▲ Previous

How to spot a planet

We can take a good guess at the number of alien Earths thanks to NASA's Kepler space telescope.
When a planet passes in front of its parent star, it blocks some of the star's light. The Kepler telescope looked for distant worlds by measuring this dip in stars' glow.

signal ▼ Next▲ Previous

In the frame

Kepler focused its gaze on the area of sky marked out by this grid of squares near the constellation Cygnus.
The telescope's detectors were trained on some 150,000 target stars in this grid for nearly four years until the end of its active planet-hunting days in May 2013.
▼ Next▲ Previous

Kepler's haul

The green dots show the possible planets discovered in Kepler's data so far.
To pursue our quest, we must exclude planets that are nothing like our home world. First, let's remove everything twice the diameter of Earth or larger, which are likely to be gas giants like Jupiter and Saturn.
▼ Next▲ Previous

In the Goldilocks zone?

The remaining planets are the right size, but not all of them will be ripe for life, with life-sustaining liquid water.
We can't determine a planet's composition from Kepler's data, but we can see whether a planet seems to orbit in the habitable zone around its parent star.

habitable_zone ▼ Next▲ Previous

These might be like home

This is our best estimate for the number of potentially life-bearing worlds among the planets spotted by Kepler. But we're missing much of the picture.
Kepler could spot only planets that passed between their parent stars and the telescope's viewpoint – even a slight tilt in a planet's orbit could make it invisible to the telescope. And the farther out a planet orbits, the more likely it was to be missed.
tilt ▼ Next▲ Previous

Earths galore

After extrapolating for all the missing worlds, Kepler's field of view becomes dense with planets that may be like Earth.
Now consider this: Kepler observed just 0.28 per cent of the sky. And the telescope was able to peer out to only 3000 light years away, studying less than 5 per cent of the stars in its field of view. So how many Earths might really be out there?
▼ Next▲ Previous

A crowded galaxy

Expanding our view from Kepler's corner of the galaxy to show more of the Milky Way, the sky fills with billions of potentially life-bearing worlds. If we showed them all, the sky would be a mass of green. So now the green dots illustrate stars that might host such planets, visible with a good pair of binoculars on a dark night here on Earth.
From this perspective, the chances that we're alone in the cosmos seem very slim, indeed.
▼ Next▲ Previous

The search continues

The Kepler telescope may no longer be hunting for alien Earths, but more discoveries are sure to come as researchers work through the backlog of data it gathered. In 2017, the search will be taken up by the Transiting Exoplanet Survey Satellite, which will survey nearby stars across the entire sky.
▼ Next▲ Previous

Credits

Thanks to Natalie Batalha, Jon Jenkins and other members of the Kepler mission team for technical advice.
Learn more about the data used in this graphic.
Produced by Adam Becker, MacGregor Campbell and Peter Aldhous.
Published 25 September 2013.
⇧ Back to top ▲ Previous

Friday, 15 August 2014

Specks returned from space may be alien visitors

Scientists say seven microscopic particles collected by NASA’s comet-chasing spacecraft, Stardust, appear to have originated outside our solar system.

A dust particle is seen on impact on a collection panel. Scientists say NASA's comet-chasing spacecraft, Stardust, may have collected the world’s first sampling of contemporary interstellar dust.
Science via Stardust ISPE / THE ASSOCIATED PRESS
A dust particle is seen on impact on a collection panel. Scientists say NASA's comet-chasing spacecraft, Stardust, may have collected the world’s first sampling of contemporary interstellar dust.
CAPE CANAVERAL, FLA.—There may be itsy-bitsy aliens among us.
Scientists say seven microscopic particles collected by NASA’s comet-chasing spacecraft, Stardust, appear to have originated outside our solar system. If confirmed, this would be the world’s first sampling of contemporary interstellar dust.
“They are very precious particles,” the team leader, physicist Andrew Westphal of the University of California, Berkeley, said in a statement Thursday.
The dust collectors were exposed to what is believed to be the interstellar dust stream in the early 2000s and returned to Earth in 2006. Since then, dozens of scientists worldwide led by Westphal have examined scans of the collection panels to zero in on the particles. The team was assisted by 30,000 citizen-scientists, dubbed Dusters, who reviewed more than 1 million images in search of elusive tracks made by incoming particles.
The findings were published Thursday in the journal Science.

Westphal said the suspected interstellar particles are surprisingly diverse. Some are fluffy like snowflakes.
A few particles splatted a little when they hit the collection panels because of their speed and the fact that some ended up hitting the aluminum foils between the softer aerogel tiles meant to capture the grains. In fact, one particle believed to be following the flow of interstellar wind was vapourized because it was going so fast — an estimated 16 kilometres per second.
The dust is considered young by cosmic standards: less than 50 million to 100 million years old, the life expectancy of interstellar dust.
Westphal said additional testing is needed before concluding these seven specks are truly from outside our solar system. And there may be more: Roughly half the dust-collection panels have yet to be scanned. The physicist expects to find no more than a dozen interstellar dust specks in all, however, a tiny fraction of the amount of comet matter gathered by Stardust.
More than 50 grains embedded in the Stardust collectors were deemed to be debris from the spacecraft itself.
NASA launched Stardust in 1999 to collect debris from Comet Wild-2. The Stardust capsule parachuted back to Earth, landing in the Utah desert seven years later.


 






Today, an astronomer is a scientist who studies celestial bodies and systems. The study of astronomy has not always been considered science nor has it always been legal. There was a time that practicing astronomy could get you tortured or killed for heresy. Today, professional astronomers are highly educated individuals. They usually have a PhD in physics or astronomy and are employed by research institutions or universities. The majority of their time is spent on research, but quite often they have additional duties like teaching, building instruments, or aiding in the operation of an observatory. The American Astronomical Society, the major organization of professional astronomers in North America, has approximately 7,700 members. This includes scientists from other fields such as physics, geology, and engineering who have research interests related to astronomy. The International Astronomical Union has 9,259 members from 89 different countries who are involved in astronomical research at the PhD level.
In ancient times, astronomy was practiced by philosophers who attempted to explain the workings of the observable night sky. This resulted in a view of the universe with the Earth at the center (geocentrism). Later, religious leaders believed that geocentrism was supported by the Bible and to argue differently was to speak against god and; therefore, heresy for which you could be tortured or put to death. Many think that modern astronomy did not develop until Galileo began his research.
Unlike the age-old image of an old astronomer peering through a telescope during the dark hours of the night, modern astronomers use a charge-coupled device (CCD) camera, which allows a more sensitive image to be created. Before CCDs, photographic plates were commonly used for observation. Modern astronomers spend little time with telescopes, maybe a few weeks per year observing. The rest of their time is spent changing data from raw to processed images, then analyzing it. Some astronomers work entirely from data.
It is hard to imagine that an area of study that has impacted our understanding of the universe around us used to be hated by the churches of the world. It is also difficult to fathom the impact a discovery by an astronomer may have on our future.

Thursday, 14 August 2014

Monster Hawaii Telescope Construction Begins

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The construction phase of the world’s biggest optical telescope has begun atop Mauna Kea, Hawaii.
Final approval by the Hawaii Board of Land and Natural Resources for a sublease on July 25 has green-lighted building work for the Thirty Meter Telescope (TMT) to begin in October.
NEWS: Monster Hawaiian Telescope Approved
With a primary mirror spanning 30 meters, the TMT will dwarf all optical telescopes on Earth and in space. The twin-telescope Keck Observatory is the next biggest telescope on Mauna Kea with mirrors measuring 10 meters across. Not only will the TMT dwarf Keck, it will also be able to acquire observations 12-times sharper than the Hubble Space Telescope.
Initiated ten years ago by the Association of Canadian Universities for Research in Astronomy (ACURA), the California Institute of Technology (Caltech) and the University of California, the TMT’s international scope has expanded to include partners around the globe. Chinese and Japanese institutions are working to build components for the TNT and India is also expected to join the collaboration.
PHOTOS: Cosmic Hotshots from Keck Observatory
“Design of the fully articulated main science steering mirror system in the telescope, as well as development of the lasers, laser guide star systems and other high-tech components, is proceeding in China,” said Yan Jun, Director General of the National Astronomical Observatories of China, in a TNT press release.
“Japan has seen to the production of over 60 mirror blanks made out of special zero-expansion glass that does not alter its shape with temperature changes,” said Masanori Iye, TMT International Observatory Board Vice Chair and TMT Japan Representative for the National Astronomical Observatory of Japan. “The blanks will be highly polished for use in the telescope’s 30-meter diameter primary mirror. The final design of the telescope structure itself is nearing completion.”
PHOTOS: Hubble’s Latest Mind Blowing Cosmic Pictures
The TMT’s 492-segment mirror will observe the Cosmos in wavelengths from near-infrared, through optical to ultraviolet, allowing us an unprecedented view of objects in our galaxy and the first stars that were forming after the Big Bang. Like Keck, the TMT will use adaptive optics (AO) to compensate for atmospheric turbulence.
AO utilizes a powerful laser that cuts through the upper atmosphere, creating an artificial star from the telescope’s perspective, detecting turbulence. It is this turbulence that is responsible for twinkling stars — interference that can blur celestial targets for telescopes on the ground. Atmospheric aberrations can then be compensated for by rapid adjustments by each telescope segment.
But to build such a huge observatory on Hawaii, special permissions were required to ensure the structure will minimize its impact on the pristine environment. But now, with this final approval, groundbreaking is scheduled to begin in a couple of months and it is hoped that we will see the first awe-inspiring observations by 2021.