Opportunity Finds Another Big Meteorite

Another Mars meteorite seen by Opportunity. Image Credit: NASA/JPL-Caltech

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It’s amazing what a rover can find laying by the side of the road. The Mars Exploration Rover Opportunity has found a rock that apparently is another meteorite. Less than three weeks ago, Opportunity drove away from a larger meteorite called “Block Island” that the rover examined for six weeks. Now, this new meteorite, dubbed “Shelter Island,” is another fairly big rock, about 47 centimeters (18.8 inches) long, that fell from the skies. Block Island is about 60 centimeters (2 feet) across and was just 700 meters (about 2,300 feet) away from this latest meteorite find. At first look, the two meteorites look to be of a similar makeup; Opportunity found that Block Island was is made of nickel and iron.

This image was taken during Oppy’s 2,022nd Martian day, or sol, (Oct. 1, 2009).

See below for a 3-D version of this image created by Stu Atkinson.

Shelter Island in 3-D.  Dimensionalized by Stu Atkinson
Shelter Island in 3-D. Dimensionalized by Stu Atkinson

Nebula Pictures

Omega Nebula

Here are some cool nebula pictures taken by the Hubble Space Telescope.

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This is a cool picture of the Omega Nebula, which is also known as the Swan Nebula, or M 17. It’s located in the constellation Sagittarius, located about 5,000 light-years from Earth.


Cat's Eye Nebula
Cat's Eye Nebula

This is picture of the Cat’s Eye Nebula, a planetary nebula in the constellation Draco. This used to be a star similar to our Sun, but then it died and became a white dwarf, puffing off its outer layers into space.


Carina Nebula
Carina Nebula

This is the Carina Nebula, a star forming nebula in the Carina Constellation. It holds Eta Carinae, one of the most massive stars ever discovered, which is expected to detonate as a supernova in the next few hundred thousand years.


Bubble Nebula. Image credit: Hubble
Bubble Nebula. Image credit: Hubble

This is the Bubble Nebula, also known as NGC 7635. This nebula glows because of a hot central star that’s providing radiation and exciting the nebula atoms.


Full view of the Trifid Nebula.  Credit: ESO
Full view of the Trifid Nebula. Credit: ESO

This is a picture of the Trifid Nebula taken by the European Southern Observatory. This nebula was cataloged M 20 by Charles Messier as part of his famous catalog. It’s called the “Trifid Nebula”, because it appears to be broken up into three parts.

We have written many stories about nebulae for Universe Today. Here’s an article with more details about the Trifid Nebula, and here’s an article about planetary nebulae found around heavy stars.

If you want more cool pictures of nebula, you should check out the source. Go to the Hubble Space Telescope page on nebulae.

We have recorded an entire episode of Astronomy Cast that’s just about nebulae. Listen here, Episode 111: Nebulae.

International Space Station Viewing

The ISS. Credit: NASA

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Now that it’s mostly complete, the International Space Station is the brightest human-built object in space. It’s easy to see with your own eyes, the trick is knowing when to step outside and look up to see the station go overhead. If you do get your timing right, you’ll see the station as a bright star moving quickly in the sky. It only take a couple of minutes to pass through the sky above your house. Want to see the station for yourself? Here are some resources for International Space Station viewing.

The best place to go is NASA’s Human Spaceflight tracking page. This shows you the current location of the International Space Station, the Hubble Space Telescope, and any space shuttles currently in orbit.

So that shows you where the space station and shuttles are right now, but how will you know when they’re going to be passing over your part of the Earth?

NASA has a page for sighting opportunities. You can either choose your location from a list of common locations around the world, or you download an application that lets you pick your specific spot on Earth. It will then tell you the exact times ISS will be passing overhead.

If you’ve got an iPhone, check out the ISS Visibility App. This tool will calculate the next times you’ll be able to see the ISS pass overhead.

You can also use a great service called Heavens Above. This will also show you the current location of satellites, as give you times when ISS will be passing overhead.

We have written many articles about the International Space Station for Universe Today. Here’s an article about how ISS is now visible in the daytime.

We have recorded an episode of Astronomy Cast about the space shuttle. Listen to it here, Episode 127: The US Space Shuttle.

Tourists to ISS Two at a Time Starting 2012?

Space Adventures logo. Credit: Space Adventures

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According to a Russian official, the commercial space company Space Adventures will be sending two space tourists a year into orbit on Soyuz spacecraft from beginning in 2012. “We have been working on this project for a number of years” said Sergey Kostenko, the head of the company’s office in Russia, who was quoted in the Russian news website RiaNovosti. “Each Soyuz will carry two tourists and a professional astronaut. One of the tourists will have to pass a year-and-a-half training course as a flight engineer.”

Space Adventures has been authorized by the Russian Federal Space Agency Roscosmos to select and contract candidates for space tourist trips. According to Kostenko, Russia’s RSC Energia corporation has the capacity to build five Soyuz spacecraft per year instead of four, meaning that Space Adventures will be able to use at least one Soyuz for space tourism purposes.

“The International Space Station (ISS) program requires four Soyuz spacecraft per year, and we have been informed by RSC Energia that they will be able to increase the annual production to five spacecraft,” he said, adding that Space Adventures would pay for the construction of the extra Soyuz, the launch services and the salary of a Russian cosmonaut as crew commander.

Kostenko said Space Adventrues, which bills itself as the only company currently providing human space mission opportunities to the world marketplace, already had a number of candidates who were willing to pay for trips into space, including Russian-born American billionaire and Google co-founder Sergey Brin.

The current price of a 10-day trip to the ISS for a tourist is estimated at about $35 million USD.

Guy Laliberte prior to his flight to the ISS.
Guy Laliberte prior to his flight to the ISS.

Space tourists started flying to the International Space Station in 2001 when American businessman and former NASA scientist Dennis Tito flew to the ISS aboard a Soyuz. He was followed by South African computer millionaire Mark Shuttleworth in 2002, and Gregory Olsen, a U.S. entrepreneur and scientist, in 2005.
In 2006, Anousheh Ansari, a U.S. citizen of Iranian descent, became the first female space tourist.

U.S. games developer Richard Garriott, the son of former NASA astronaut Owen K. Garriott, went into orbit for 11 days in October 2008 on board a Russian Soyuz TMA-13.

U.S. space tourist Charles Simonyi, one of the founders of Microsoft, made two trips to the ISS – in 2005 and 2009.

Guy Laliberte, the Canadian founder of entertainment company Cirque du Soleil, arrived at the ISS on Friday and will stay on board until October 10.

Source: Ria Novosti

Weekend SkyWatcher’s Forecast – October 2-4, 2009

Greetings, fellow SkyWatchers! Are you ready to catch the planetary action? Then get thee out into the night, because right now is the perfect time of year to catch all of our solar system bodies in the same day! Be sure to be out on Saturday night, too… Because it’s “Harvest Moon”! Need a little bit more of a challenge? Then fly off to Cygnus as we take a look at two of its most beautiful (and challenging) double stars! Whenever you’re ready, I’ll see you in the dark…

solarsystemFriday, October 2, 2009 – It’s that time of year! Time to be able to see all the planets in 24 hours! If you’re able to get up before sunrise, it’s a good time to watch celestial mechanics in action as Mercury, Venus, and Saturn are beginning to draw together just before dawn. Be on the lookout for Mars nearly overhead. Now is a good time to see details.

If you haven’t spotted Uranus yet, let the Moon be your guide tonight for finding it about 5 degrees south. Even with bright skies, you should be able to distinguish its faint greenish disk from surrounding stars. What of Neptune? The blue world is a bit further from the Moon tonight on the ecliptic, and you’ll find it around 21:45 in right ascension. The last is the mighty Jove. For binoculars and telescopes, Jupiter is definitely the king of the observable planets for detail. Not only can you spot its different zones and equatorial belts, but refractor users can also regularly distinguish the faded Great Red Spot and other fine features, such as white ovals. For all larger apertures, be on the lookout for the moons! It’s very exciting to watch a shadow transit or to catch a Galilean as it reappears from behind the limb. In just a matter of a few hours, Jupiter’s details can change greatly!

For those who still cheer for Pluto’s status as a planet? The tiny god of the underworld still holds its place in our Solar System. . .and the sky! You can find it during the early evening around 18:02 in right ascension. Good luck on your planet quest!!

Saturday, October 3, 2009 – When the Universal Date changes tonight, the Moon will become full, and this will be the one closest to the autumnal equinox. Because the Moon’s orbit is more nearly parallel to the eastern horizon, it will rise near dusk for the next several nights in a row. On the average, the Moon rises about 50 minutes later each night, but at this time of year it’s around 20 minutes later for mid-northern latitudes and even later further north. Because of this added light, the name ‘‘Harvest Moon’’ was coined; it allowed farmers more time to work in the fields.

smoon

Often times we perceive the Harvest Moon as being more orange than at any other time of the year. The coloration is caused by the scattering of the light by particles in our atmosphere. When the Moon is low, like now, we get more of that scattering effect, and it truly does appear more orange. The very act of harvesting itself produces more dust, and often times that coloration will last the whole night through. And we all know the size is only an ‘‘illusion’’. . .

So, instead of cursing the Moon for hiding the deep-sky gems tonight, enjoy it for what it is, a wonderful natural phenomenon that doesn’t even require a telescope!

sputnik1Sunday, October 4, 2009 – This date in 1957, the USSR’s Sputnik 1 made space history, as it became the first man-made object to orbit Earth. Earth’s first artificial satellite was tiny, roughly the size of a basketball, and weighed no more than the average man. Every 98 minutes it swung around Earth in its elliptical orbit. . .and changed everything. It was the beginning of the ‘‘Space Age.’’ Take the time with your children or grandchildren to check Heaven’s Above for visible passes of the International Space Station (ISS), and think about how much our world has changed in just over half a century!

Tonight we’ll begin with an easy double star and make our way toward a more difficult one. Beautiful, bright, and colorful, Beta Cygni is an excellent example of an easily split double star.

betacygni

As the second brightest star in the constellation of Cygnus, Albireo lies roughly in the center of the ‘‘Summer Triangle,’’ making it a relatively simple target for even urban telescopes. Albireo’s primary (or brightest) star is around magnitude 4 and has a striking orangish color. Its secondary (or B) star is slightly fainter at a bit less than magnitude 5, and often appears to most as blue, almost violet. The pair’s wide separation of 3400 makes Beta Cygni an easy split for all telescopes at modest power, and even for larger binoculars. At approximately 410 light-years away, this colorful pair has a separation of about 4,400 Astronomical Unit (AU). As Burnham noted:

‘‘It is worth contemplating, in any case, the fact that at least 55 Solar Systems could be lined up, edge-to-edge, across the space that separates the components of this famous double!’’

deltacygniNow let’s have a look at Delta (RA 19 44 58 Dec +45 07 50). Located around 270 light-years away, Delta is a more difficult binary star. Its duplicity was discovered by F. Struve in 1830, and it is a very tough test for smaller optics. Located no more than 220AU away from the magnitude 3 parent star, the companion takes anywhere from 300 to 540 years to orbit its star and is often rated as dim as 8th magnitude. If skies aren’t steady enough to split it tonight, try again! Both Beta and Delta are on many challenge lists.

Until next week? Ask for the Moon… But keep on reaching for the stars!

This week’s awesome images are (in order of appearance): Solar System Montage (credit—NASA), Saguaro Moon (credit and copyright—Stefan Seip (NASA/APOD), Sputnik Archival Image, Beta Cygni: Albireo (credit—University of Nebraska-Lincoln) and Delta Cygni (credit—Palomar Observatory, courtesy of Caltech). We thank you so much!

1 AU in KM

Earth from space

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1 AU in KM = 149,598,000 kilometers

An astronomical unit is a method that astronomers use to measure large distances in the Solar System. 1 astronomical unit, or 1 au, is the average distance from the Sun to the Earth.

The Earth’s orbit around the Sun is actually elliptical. It varies from 147 million km to 152 million km. So the measurement of an astronomical unit is just the Earth’s average distance from the Sun. That’s where the more precise measurement of 1 AU to KM (149,598,000 km) comes from.

Here are some other distances in the Solar System:
Mercury: 0.39 AU
Venus: 0.72 AU
Mars: 1.5 AU
Jupiter: 5.2 AU
Saturn: 9.6 AU
Uranus: 19.2 AU
Neptune: 30.1 AU
Pluto: 39.5 AU
Eris: 67.7 AU
Oort Cloud: 50,000 AU
Alpha Centauri: 275,000 AU

We have written many articles about large distances in space. Here’s an article that explains how far space is, and here’s an article about the distance to stars.

You can also check out this cool calculator that lets you convert astronomical units into any other distance.

We have also recorded an episode of Astronomy Cast detailing how astronomers measure distance in the Universe. Check out Episode 10: Measuring Distance in the Universe.

Busy Space Station: 3 Soyuz Now Docked to ISS

One of three Soyuz docked to ISS. Credit: NASA

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The International Space Station is taking on the look and feel of a busy space way station, with three Soyuz now docked and a current crew count of nine. Expedition 21 Flight Engineers Jeff Williams and Maxim Suraev along with spaceflight participant Guy Laliberté arrived at the ISS, docking their Soyuz TMA-16 to the aft end of the Zvezda service module at 4:35 a.m. EDT Friday. Williams and Suraev are relieving Expedition 20 Commander Gennady Padalka and Flight Engineer Michael Barratt who will depart on Oct. 10 along with the Canadian visitor, Laliberté (the one with the clown nose, below). Watch the docking video below, along with another video of the hatch opening and the new crew members entering the station.

Herschel Sees Hidden Stars in the Southern Cross

Herschel sees a reservoir of cold gas in the constellation of the Southern Cross. Credit: ESA

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Science observations have begun in earnest for the Herschel Space Telescope, and this spectacular image is the first produced by combining data from two cameras aboard Herschel, the Spectral and Photometric Imaging REceiver (SPIRE), and the Photoconductor Array Camera and Spectrometer (PACS). It shows a tumultuous region in the Southern Cross, visible only because the instruments are tuned to “see” in five different infrared wavelengths. Stunning vistas of cold gas clouds lying near the plane of the Milky Way reveal intense, unexpected activity. The dark, cool region is dotted with stellar factories, like pearls on a cosmic string.

Herschel, one of the largest telescopes in space, was launched in May. For this image, the two instruments were aimed at an area in the plane of the Milky Way about 60° from its center. It covers around 16 times the area of the Full Moon as seen in the sky.

The images were taken on September 3, 2009 during the first trial run with the two instruments working together. Herschel will go on to survey large areas of our galaxy.

Herschel SPIRE (left) and PACS images.  Credit:  ESA
Herschel SPIRE (left) and PACS images. Credit: ESA

The five original infrared wavelengths have been color-coded to allow scientists to differentiate extremely cold material (red) from the surrounding, slightly warmer stuff (blue).

The images reveal structure in cold material in our Galaxy, as we have never seen it before, and even before a detailed analysis, scientists have gleaned information on the quantity of the material, its mass, temperature, composition and whether it is collapsing to form new stars.

Beautiful evidence that our galaxy keeps giving birth to new generations of stars!

Source: ESA

Ig Nobel Prizes Awarded for 2009

The Ig Nobel awards. Credit: Harvard University

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Ahh, the wonders of science! But some science is just a little more wonderful than others. For the really great and wonderful science there are the Nobel Prizes. For the off-the-beaten-path and unusual science, Harvard University’s Annals of Improbable Research magazine awards the “Ig Nobel” Prizes, touted as “research that makes people laugh and then think.” Prizes were doled out Oct. 1, but if you are in the Massachusetts area, you might want to attend a free lecture given by the winners on Oct. 3 at 1:00 pm EDT. Here are the 2009 winners:

Veterinary medicine: Catherine Douglas and Peter Rowlinson for showing that cows with names give more milk than unnamed cows.

Peace: Stephan Bolliger, Steffen Ross, Lars Oesterhelweg, Michael Thali and Beat Kneubuehl for investigating whether it is better to be struck over the head with a full beer bottle or with an empty beer bottle.

Economics: Executives of four Icelandic banks for showing how tiny banks can become huge banks, and then become tiny banks again.

Chemistry: Javier Morales, Miguel Apatiga and Victor Castaño for creating diamonds out of tequila.

Medicine: Donald Unger for cracking just the knuckles on his left hand for 60 years to see whether knuckle-cracking contributes to arthritis.

Physics: Katherine Whitcome, Liza Shapiro and Daniel Lieberman for figuring out why pregnant women don’t tip over.

Literature: The Irish national police for issuing 50 tickets to one Prawo Jazdy, which in Polish means “driver’s license.”

Public health: Elena Bodnar, Raphael Lee and Sandra Marijan for inventing a brassiere than can be converted into a pair of gas masks.

Mathematics: Gideon Gono and the Zimbabwean Reserve Bank for printing bank notes in denominations from 1 cent to $100 trillion.

Biology: Fumiaki Taguchi, Song Guofu and Zhang Guanglei for demonstrating that bacteria in panda poop can help reduce kitchen waste by 90%.

Source: Annals of Improbable Research.

More New Looks at Mercury from MESSENGER

Bright spot on Mercury. Credit: NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington

[/caption]More new images were released today from the MESSENGER spacecraft’s third flyby of Mercury. I asked astrophysicist Dr. Jeff Goldstein (doctorjeff on Twitter), (who was on hand at the mission operations center to blog and Tweet about the flyby) which image the science team found most intriguing, and he replied that it was really hard to tell, as they were oohing and aahing at every image! But one of the most interesting was this shot of a bright spot on the planet closest to the sun. MESSENGER’s Narrow Angle Camera also saw this spot during the spacecraft’s second Mercury flyby on October 6, 2008, but the bright feature was just on the planet’s limb (edge) from the spacecraft’s vantage point. This time, however, the geometry of MESSENGER’s flyby provided a better look at this feature. Surprisingly, at the center of the bright halo is an irregular depression, which may have formed through volcanic processes. Color images from MESSENGER’s Wide Angle Camera reveal that the irregular depression and bright halo have distinctive color. This area will be of particular interest for further observation during MESSENGER’s orbital operations starting in 2011.

Craters form a paw print on Mercury. Credit: NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington
Craters form a paw print on Mercury. Credit: NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington

If you like seeing a little pareidolia, here’s a fun one: a paw print! Mercury’s surface is covered with craters in many sizes and arrangements, the result of impacts that have occurred over billions of years. In the top center of the image, outlined in a white box and shown in the enlargement at upper right, is a cluster of impact craters on Mercury that appears coincidentally to resemble a giant paw print. In the “heel” are overlapping craters, made by a series of impacts occurring on top of each other over time. The four “toes” are single craters arranged in an arc northward of the “heel.” The “toes” don’t overlap so it isn’t possible to tell their ages relative to each other. The newly identified pit-floor crater can be seen in the center of the main image as the crater containing a depression shaped like a backward and upside-down comma.

For more of the latest images from the third flyby, check out the MESSENGER flyby page.