Galaxy M60-UCD1 is an ultra-compact dwarf galaxy, and is packed with an extraordinary number of stars. Credit: X-ray: NASA/CXC/MSU/J.Strader et al, Optical: NASA/STScI
Meet galaxy M60-UCD1. This is not your average, every day, ordinary galaxy. First of all, it’s what is known as an ‘ultra-compact dwarf galaxy,’ which – as the name implies — are unusually dense and small galaxies. Additionally, it is the most luminous known galaxy of its type and one of the most massive, weighing 200 million times more than our Sun. But M60-UCD1 is jam-packed with an extraordinary number of stars, making it the densest galaxy in the nearby Universe that we know of. Stars in M60-UCD1 are thought to be 25 times closer together than the stars in our galaxy.
Quick and easy access to neighboring star systems (if you lived there) might be your first thought. But remember, space is big, no matter where you are.
“Traveling from one star to another would be a lot easier in M60-UCD1 than it is in our galaxy,” said Jay Strader of Michigan State University in Lansing, first author of a paper describing these results. “But it would still take hundreds of years using present technology.”
Ultra-compact dwarf galaxies were discovered about a decade ago. They are typically about only 100 light years across compared to the 1,000 light years or more than other dwarf galaxies. Our Milky Way galaxy is 120,000 light-years across.
This graph shows where M60-UCD1 fits in as far as luminosity and size. Credit: Strader et al.
Strader said that what makes M60-UCD1 so remarkable is that about half of its mass is found within a radius of only about 80 light years. This would make the density of stars about 15,000 times greater than found in Earth’s neighborhood in the Milky Way.
“Our discovery of M60-UCD1 lends support to the idea that ultra-compact dwarfs could be stripped-down version of more massive galaxies,” Strader wrote in a post on the Chandra blog. “The first reason is its mass: we estimate that it contains about 400 million stars, far more than observed for even massive star clusters, and much closer to the galaxy regime. We also observe that M60-UCD1 has two “parts”: an inner, even denser core embedded in a more diffuse field of stars. This structure is not expected for a star cluster, but it’s a natural outcome of the tidal stripping process that could produce an ultra-compact dwarf.”
And so, this UCD is providing astronomers with clues to how these types of galaxies fit into the galactic evolutionary chain.
Additionally, this galaxy appears to have a central black hole, as Chandra X-ray Observatory reveal the presence of an X-ray source sitting right at the center.
While supermassive black holes are known to be common in the most massive galaxies, it is unknown whether they occur in less massive galaxies like M60-UCD1, Strader said.
“Further observations of M60-UCD1 and other ultra-compact dwarfs could confirm a new, significant population of massive black holes,” Strader said. “These masses of these black holes would be notable: while most central black holes in galaxies have only a fraction of a percent of the mass of their host galaxies, in ultra-compact dwarfs the black holes could be a full 10% of the mass of the dwarf. This is because so many of the dwarf’s outer stars have been stripped away, essentially boosting the contribution of the unaffected central black hole to the total mass of the galaxy.”
M60-UCD1 is located near a massive elliptical galaxy NGC 4649, also called M60, about 60 million light years from Earth. The galaxy was discovered with NASA’s Hubble Space Telescope and follow-up observations were done with NASA’s Chandra X-ray Observatory, the Keck Observatory in Hawaii, and the Multiple Mirror Telescope in Arizona.
This view of Saturn's moon Enceladus and its prominent plumes was taken by the Cassini spacecraft on April 2, 2013. Credit: NASA/JPL-Caltech/Space Science Institute.
We can never get enough of seeing those intriguing jets and plumes from Saturn’s moon Enceladus, especially this great view from the Cassini spacecraft where the plumes are back-it from the Sun while the moon’s surface is lit with reflected light from Saturn. And as you can see, those jets are still firing. There are close to 100 geyser jets of varying sizes near Enceladus’s south pole spraying water vapor, icy particles, and organic compounds out into space. If you look closely, you’ll see the entire plume is as large as the moon itself.
Can we please send another spacecraft just to study this fascinating moon?
The image was taken in blue light with the Cassini spacecraft narrow-angle camera on April 2, 2013, when Cassini was about 517,000 miles (832,000 kilometers) from Enceladus.
A Soyuz rocket is rolled out to the launch pad by train on Monday, Sept. 23, 2013, at the Baikonur Cosmodrome in Kazakhstan. Credit: NASA/Carla Cioffi.
A new Soyuz is now on the pad, ready to bring the next crew to the International Space Station. Launch is scheduled for at 20:58 UTC (4:58 p.m. EDT) on September 25. This is the third Soyuz spacecraft to use the new abbreviated rendezvous trajectory with the ISS, where it will reach the space station in just a few hours instead of the usual two days.
Below is a video of the rollout to the pad.
You can see a great collection of images from the rollout, a press conference and more from NASA HQ’s Flickr page.
This Soyuz rocket will send Expedition 37 Soyuz Commander Oleg Kotov, NASA Flight Engineer Michael Hopkins and Russian Flight Engineer Sergei Ryazansky on a five-and-a-half month mission aboard the International Space Station.
In the past, Soyuz manned capsules and Progress supply ships were launched on trajectories that required about two days, or 34 orbits, to reach the ISS. For tomorrow’s launch, the Soyuz will rendezvous with the space station and dock after four orbits of Earth. The new fast-track trajectory has the rocket launching shortly after the ISS passes overhead. Then, additional firings of the vehicle’s thrusters early in its mission expedites the time required for a Russian vehicle to reach the Station.
Docking to the Poisk module on the Russian segment of the station is expected to occur at 02:47 UTC on Sept. 26 (10:47 p.m. EDT, Sept. 25) All the action of the launch and docking will be on NASA TV.
The new crew will join the current Expedition 37 crew of Commander Fyodor Yurchikhin, Karen Nyberg and Luca Parmitano of the European Space Agency.
Hopkins, Kotov and Ryazanskiy will remain aboard the station until mid-March. Yurchikhin, Nyberg and Parmitano, who have been aboard the orbiting laboratory since late May, will return to Earth Nov. 11, leaving Kotov as commander of Expedition 38.
The entire disk of the Earth lit during the equinox on September 22, 2013. Credit: Roscosmos / NTSOMZ / SRC "Planeta" / zelenyikot.livejournal.com
Here’s a fantastic view of our home planet taken by the Russian weather satellite Electro-L. And while Elektro-L can take gigantic photographs of the entire planet every 30 minutes, it only can get a fully-lit view like this just twice a year — at the spring and autumn equinoxes. This image was taken during the autumnal equinox on September 22, 2013.
Below is an animated gif of the view, going from day to night.
Animation of the Electro-L satellite’s view of Earth on September 22, 2013. Credit: Roscosmos / NTSOMZ / SRC “Planeta” / zelenyikot.livejournal.com
Elektro-L orbits Earth in a geostationary orbit 36,000 kilometers above the equator, and with the Sun exactly behind the satellite on the equinox — the day the north and south poles get the same amount of light — the entire disk is fully lit.
You can see the typhoon Usagi raging over Southeast Asia, clouds and rain over Russia and swirling clouds in the ocean near Antarctica.
Electro-L was launched in 2011 and is Russia’s first geostationary weather satellite. It’s a data hog – sending back 2.56 to 16.36 megabits per second, with resolution of 1 kilometer per pixel. You can see the big 5000 x 5000 pixel version at the Electro-L website.
Thanks to Vitaliy Egorov for sharing this image with UT. He has posted the images at his zelenyikot/livejournal website.
An oblique view of pyroclastic vents on Mercury via MESSENGER
Here on Earth we’re used to seeing volcanoes as towering mountains with steam-belching peaks or enormous fissures oozing lava. But on Mercury volcanic features often take the form of sunken pits surrounded by bright reflective material. They look like craters from orbit but are more irregularly-shaped, and here we have a view from MESSENGER of a cluster of them amidst a rugged landscape that stretches all the way to the planet’s limb.
The image above shows a group of pyroclastic vents on Mercury, located just north and east of the 180-mile (290-km) -wide, double-ringed Rachmaninoff crater. The vents lie in the center of a spread of high-reflectance material, sprayed out by ancient eruptions. This bright blanket of material stands out against Mercury’s surface so well, it has even been spotted in Earth-based observations!
An older vent can be seen at the bottom right, looking like a crater but with non-circular walls. North is to the left.
So why do Mercury’s volcanoes look so different than Earth’s? Planetary scientist David Blewett from Johns Hopkins University Applied Physics Laboratory explains:
“Volcanism on Mercury (and also the Moon) appears to have been dominated by flood lavas, in which large quantities if highly fluid (low-viscosity) magma erupts and flows widely to cover a large area. In this type of eruption, no large ‘volcano’ edifice is constructed,” David wrote in an email. “The lunar maria and many of Mercury’s smooth plains deposits were formed in this manner.”
“On both the Moon and Mercury there are also examples of explosive activity in which eruptions from a vent showered the surroundings with pyroclastic material (volcanic ash),” he added. “The vents and bright pyroclastic halos seen near Rachmaninoff on Mercury are examples, as well as numerous ‘dark mantle deposits’ on the Moon.”
The discovery and investigation of vents like these is extremely valuable to scientists, as they provide information on Mercury’s formation, composition, and the nature of volatiles in its interior. (Plus the oblique angle is very cool! Makes you feel like you’re flying along with MESSENGER over Mercury’s surface.)
See below for a wider view of the region and context of the placement of these vents to Rachmaninoff.
MESSENGER image of Rachmaninoff crater obtained in September 2009
We’re in the middle of Summer here on Vancouver Island, the Sun is out, the air is warm, and the river is great for swimming.
Three months from now, it’s going to be raining and miserable.
Six months from now, it’s still going to be raining, and maybe even snowing.
No matter where you live on Earth, you experience seasons, as we pass from Spring to Summer to Fall to Winter, and then back to Spring again.
Why do we have variations in temperature at all? What causes the seasons?
If you ask people this question, they’ll often answer that it’s because the Earth is closer to the Sun in the summer, and further in the winter.
But this isn’t why we have seasons. In fact, during Winter in the Northern Hemisphere, the Earth is actually at the closest point to the Sun in its orbit, and then farthest during the Summer. It’s the opposite situation for the Southern hemisphere, and explains why their seasons are more severe.
So if it’s not the distance from the Sun, why do we experience seasons?
We have seasons because the Earth’s axis is tilted.
Consider any globe you’ve ever used, and you’ll see that instead of being straight up and down, the Earth is at a tilt of 23.5-degrees.
The Earth’s North Pole is actually pointed towards Polaris, the North Star, and the south pole towards the constellation of Octans. At any point during its orbit, the Earth is always pointed the same direction.
For six months of the year, the Northern hemisphere is tilted towards the Sun, while the Southern hemisphere is tilted away. For the next six months, the situation is reversed.
Whichever hemisphere is tilted towards the Sun experiences more energy, and warms up, while the hemisphere tilted away receives less energy and cools down.
Consider the amount of solar radiation falling on part of the Earth.
When the Sun is directly overhead, each square meter of Earth receives about 1000 watts of energy.
But when the Sun is at a severe angle, like from the Arctic circle, that same 1000 watts of energy is spread out over a much larger area.
This tilt also explains why the days are longer in the Summer, and then shorter in the Winter.
The longest day of Summer, when the Northern Hemisphere is tilted towards the Sun is known as the Summer Solstice.
And then when it’s tilted away from the Sun, that’s the Winter Solstice.
When both hemispheres receive equal amounts of energy, it’s called the Equinox. We have a Spring Equinox, and then an Autumn Equinox, when our days and night are equal in length.
So how does distance from the Sun affect us?
The distance between the Earth and has an effect on the intensity of the seasons.
The Southern Hemisphere’s Summer happens when the Earth is closest to the Sun, and their winter when the Earth is furthest. This makes their seasons even more severe.
You might be interested to know that the orientation of the Earth axis is actually changing.
Over the course of a 26,000 year cycle, the Earth’s axis traces out a great circle in the sky. This is known as the precession of the equinoxes.
At the halfway point, 13,000 years, the seasons are reversed for the two hemispheres, and then they return to original starting point 13,000 years later.
You might not notice it, but the time of the Summer Solstice comes earlier by about 20 minutes every year; a full day every 70 years or so.
I hope this helps you understand why the Earth – and any planet with a tilted axis – experiences seasons.
Comet ISON, as seen on September 22, 2013 at 10:00 UTC (6:00 am EDT) from Yellow Springs, Ohio, using a QHY8 CCD camera and a home-made 16 inch diameter telescope. 15 minute exposure. Credit and copyright: John Chumack.
Perhaps you’ve read the news. This Fall, the big ticket show is the approach of Comet C/2012 S1 ISON. The passage of this comet into the inner solar system has been the most anticipated apparition of a comet since Hale-Bopp in 1997.
Many backyard observers will get their first good look at Comet ISON in the coming month. If you want to see this comet for yourself, here’s everything you’ll need to know!
A composite image of Comet ISON as seen from the Hubble Space Telescope on April 30th, 2013. (Credit: HubbleSite.org/Go/ISON).
Discovered on September 21st, 2012 by Artyom-Kislovodsk and Vitaly Nevsky using the International Scientific Optical Network’s (ISON) 0.4 metre reflector, this comet has just passed out from behind the Sun from our Earthly vantage point this summer to once again become visible in the dawn sky.
Of course, there’s much speculation as to whether this will be the “comet of the century” shining as “bright as the Full Moon” near perihelion. We caught up with veteran comet observer John Bortle earlier this year to see what skywatchers might expect from this comet in late 2013. We’ve also chronicled the online wackiness of comets past and present as ISON makes its way into the pantheon as the most recently fashionable scapegoat for “the end of the world of the week…”
But now it’s time to look at the astronomical prospects for observing Comet ISON, and what you can expect leading up to perihelion on November 28th.
Comet ISON as recently imaged by Efrain Morales on September 22nd. (Credit: Efrain Morales/Jaicoa Observatory, used with permission).
Advanced amateur astronomers are already getting good images of Comet ISON, which currently shines at around +12th magnitude in the constellation Cancer. And although NASA’s Deep Impact/EPOXI mission is down for the count, plans are afoot for the Curiosity rover and the Mars Reconnaissance Orbiter to attempt imaging the comet when it makes its closest approach to the Red Planet on October 1st at 0.0724 Astronomical Units (A.U.) or 10,830,000 kilometres distant. If MSL is successful, it would be the first time that a comet has been observed from the surface of another world.
Currently, ISON sits about a magnitude below the projected light curve, (see below) but that isn’t all that unusual for a comet. Already, there’s been increasing talk of “ISON being a dud,” but as Universe Today’s Nancy Atkinson pointed out in a recent post, these assertions are still premature. The big question is what ISON will do leading up to perihelion, and if it will survive its passage 1.1 million kilometres above the surface of the Sun on November 28th to become a fine comet in the dawn skies in the weeks leading up to Christmas.
ISON is already starting to show a short, spikey tail in amateur images. Tsutomu Seki estimated it to be shining at about magnitude +11.1 on September 16th. Keep in mind, a caveat is in order when talking about the magnitudes of comets. Unlike stars, which are essentially a point source, the brightness of a comet is spread out over a large surface area. Thus, a comet may appear visually fainter than the quoted magnitude, much like a diffuse nebula. Although +6th magnitude is usually the limit for naked eye visibility, I’ll bet that most folks won’t pick up ISON with the unaided eye from typical suburban sites until it breaks +4th magnitude or so.
The recent revised light curve projected for Comet ISON (Credit: NASA CIOC/Compiled by Matthew Knight of the Lowell Observatory).
The forward scattering of light also plays a key role in the predicted brightness of a comet. The November issue of Astronomy Magazine has a great article on this phenomenon. It’s interesting to note that ISON stacks up as a “9” on their accumulated point scale, right at the lower threshold of comet “greatness,” versus a 15 for sungrazing Comet C/1965 S1 Ikeya-Seki. Another famous “9” was Comet C/1996 B2 Hyakutake, which passed 0.1018 A.U. or 15.8 million kilometres from Earth on March 25, 1996.
ISON will pass 0.429 A.U. or 64.2 million kilometres from Earth the day after Christmas. Bruce Willis can stay home for this one.
Here is a blow-by-blow breakdown of some key dates to watch for as ISON makes its plunge into the inner solar system:
-September 25th: ISON crosses the border from the astronomical constellation of Cancer into Leo.
-September 27th: ISON passes 2 degrees north of the planet Mars.
The path of Comet ISON from October 1st to November 21st. The position of the Sun is shown on the final date. (Created by the Author using Starry Night Education software).
-October 1st: The 12% illuminated waning crescent Moon passes 10 degrees south of Mars & ISON.
-Early October: ISON may break +10th magnitude and become visible with binoculars or a small telescope.
-October 4th: New Moon occurs. The Moon then exits the dawn sky, making for two weeks of prime viewing.
–October 10th: ISON enters view of NASA’s STEREO/SECCHI HI-2A CAMERA:
-October 16th: ISON passes just 2 degrees NNE of the bright star Regulus, making a great “guidepost” to pin it down with binoculars.
-October 18th: The Full Moon occurs, after which the Moon enters the morning sky.
-October 26th: A great photo-op for astro-imagers occurs, as ISON passes within three degrees the Leo galaxy trio of M95, M96, & M105.
The position of Comet ISON on October 26th in Leo near Mars and a trio of galaxies. (Created by the author in Stellarium).
-October 30th: The 17% illuminated Moon passes 6 degrees south of ISON.
-Early November: Comet ISON may make its naked eye debut for observers based at dark sky sites.
-November 3rd: A hybrid (annular-total) solar eclipse occurs, spanning the Atlantic and Central Africa. It may just be possible for well placed observers to catch sight of ISON in the daytime during totality, depending on how quickly it brightens up. The Moon reaching New phase also means that the next two weeks will be prime view time for ISON at dawn.
-November 5th: ISON crosses the border from the astronomical constellation of Leo into Virgo.
-November 7th: ISON passes less than a degree from the +3.6 magnitude star Zavijava (Beta Virginis).
-November 8th: ISON passes through the equinoctial point in Virgo around 16:00 EDT/20:00 UT, passing into the southern celestial hemisphere and south of the ecliptic.
-November 14th: ISON passes less than a degree from the 10th magnitude galaxy NGC 4697.
-November 17th: The Moon reaches Full, passing into the morning sky.
-November 18th: ISON passes just 0.38 degrees north of the bright star Spica.
-November 22nd: ISON crosses into the astronomical constellation of Libra.
-November 23rd: ISON sits 4.7 degrees SSW of the planet Mercury and 4.9 SSW of Saturn, respectively.
Looking east before dawn on the morning of November 23rd. Note comet 2P/Encke nearby! (Created by the author using Starry Night Education software).
-November 25th: ISON pays a visit to another famous comet, passing just 1.2 degrees south of short period comet 2P/Encke which may shine at +8th magnitude.
-November 27th: ISON enters the field of view of SOHO’s LASCO C3 coronagraph.
-November 28th: ISON reaches perihelion at ~18:00 PM EST/ 23:00 UT.
After that, all bets are off. The days leading up to perihelion will be tense ones, as ISON then rounds the Sun on a date with astronomical destiny. Will it join the ranks of the great comets of the past? Will it stay intact, or shatter in a spectacular fashion? Watch this space for ISON updates… we’ll be back in late November with our post-perihelion guide!
Chinese taikonauts (from left) Liu Yang, Jing Haipeng and Liu Wang. Credit: www.news.cn
China’s human spaceflight program may soon be opening the door to foreign astronauts. The Asian nation has so far been forging ahead with a small space station and its own flights, independent of the multinational collaboration taking place with the International Space Station, although it has done work with Russia and France.
Last week, however, a Chinese official said the country is considering bringing foreign astronauts on board its spacecraft and also providing training for them.
“We would like to train astronauts from other countries and organizations that have such a demand, and we would be glad to provide trips to foreign astronauts,” said Yang Liwei, deputy director of China Manned Space Agency, in a report from China Daily.
Launch of Shenzhou 7. Credit: PR China
“We will also welcome foreign astronauts who have received our training to work in our future space station.”
Yang’s remarks came at the United Nations/China Workshop on Human Space Technology. The director also pointed out that European astronauts have visited the Chinese facilities, and vice versa, which could point the way forward to more work between the nations.
China’s most recent spaceflight took place in June. Shenzhou 10 docked with a small space station in orbit (Tiangong-1.) The country is reportedly planning a larger space station in the coming years and possibly, some manned lunar missions.
Abigail Harrison just prior to the launch of her mentor astronaut, Luca Parmitano, in Kazakhstan May 28, 2013. Credit: Abigail Harrison
Meet Abigail Harrison. This teenager’s enthusiasm about space so impressed Luca Parmitano — who just happens to be a European Space Agency astronaut on the space station right now — that the two have a social media collaboration going.
Abby collects questions from readers of her blog (AstronautAbby.com) and sends them up to the station for Parmitano to read and respond to.
Parmitano’s first mission in space, which he calls Volare (“Fly”), has been a busy one. He’s driven a rover, practiced grappling techniques for the Cygnus spacecraft — which was delayed in its docking to Tuesday (now Saturday) — and experienced two spacewalks (one went to plan, and the other was cut short due to a spacesuit leak).
Meanwhile, Abby had a space-y summer of her own. She fundraised thousands of dollars to see Parmitano’s launch in May. Then she went to Space Camp and toured several NASA and international agency centers. We caught up with Abby to find out how things are going — and if this brings her any closer to her dream of going to space herself. Below is a slightly edited e-mail conversation about her adventures.
Universe Today: How’s it going with the partnership?
Abigail Harrison: Working with Luca has been a lot of fun! I have really enjoyed being able to e-mail with him on station and especially the opportunity I had to talk to him while visiting Marshall Space Flight Center in Huntsville, AL at the end of July. The AstronautAbby community has been very active sharing images of the Space Station flying by for my #CatchLuca weekly blog post, and the #AskLuca questions submitted by my community have been great. It’s fun to hear how Luca answers these questions each week.
UT: What are the best things that you have been doing specifically to spread the message of Volare?
AH: I think my #CatchLuca blog series has been a real hit! So many people from around the world have taken photos of the ISS passing overhead and decided to submit them and share with the world. It’s been great! I think this helps to spread the message as it is people on Earth getting excited about the space station and sharing their own pictures. The more sharing that happens, the more aware people get about the mission and the more they learn.
Luca Parmitano, a European Space Agency astronaut, is on his first voyage to space as a part of Expeditions 36/37. Credit: NASA
The #AskLuca series has also been very successful. It’s true, anyone can jump on social media and ask a question of Luca or any astronaut and they most likely will answer it, but this series has allowed people who may not be socially savvy to ask questions, as well as people to ask longer questions. The fact that all the answers are published on my blog is also great as people can read it in a published article versus on a social media update.
UT: Tell us more about these NASA tours you’ve been doing lately. What is your goal in doing them?
AH: I have been fortunate to be in the right places at the right time. This summer I was in Houston for a gymnastics camp, and therefore I was able to tour the Johnson Space Center – but not just tour the center, I got to see the Neutral Buoyancy Lab and compare it to the Russian counterpart that I saw in May during my visit to Star City [astronaut training complex in Russia] when attending Luca’s launch. I also was able to go on the floor of Mission Control and see a specialized robotics lab, along with a lot of other cool things.
Abigail Harrison simulates repairing a satellite during Space Camp in Huntsville, AL. Credit: Abigail Harrison
After Houston, I headed to Huntsville for Space Camp. While in Huntsville I was able to tour the Marshall Space Flight Center and specifically see some of the work NASA is doing along with ATK to build the Space Launch System, which is the rocket system that will take me to Mars someday (similar but much bigger than the Saturn V rockets that took Apollo to the moon).
Finally, I visited Lockheed Martin’s facilities in Colorado to see the production of the Orion, which is the spacecraft currently being developed to go to Mars, the moon and asteroids. These visits have tremendous value as I have been able to share pictures, write about the visits and talk about what I have seen with people everywhere.
The goal is to learn about what is being done right now to realize the future American missions to Mars, the moon and asteroids and continue human space flight. The more I learn and understand about our current efforts to realize the future of human space exploration, the easier it is for me to talk about the future and educate the general public. Part of my mission is to help spread the word to people around the world about the future of human space flight and get the public excited for what we will do next.
Abigail Harrison with subscale test rocket motors during a visit to the Marshall Space Flight Center in Huntsville, AL. Credit: Abigail Harrison
UT: I’m sure you’ve been talking to Luca regularly. What do you talk about?
AH: We e-mail and tweet quite a bit. We have only talked once. To be honest, I follow his mission very closely through his online updates and ESA and NASA updates for my role as his Earth Liaison, and therefore I am up to date on what he is doing, probably more up to date than most people.
When we e-mail and talk it is usually about other things like advice on school, travel (he lives in Houston so gave me some good tips on what to see while visiting), and generally asking him how he is doing and what it is like to live and work on the ISS. It’s not that different from when he was training for his mission on Earth, except for now he is flying in space overhead and his e-mails and tweets come from space. 🙂
UT: Do you feel any closer to being in space as a result of this partnership?
AH: Yes, I do. How could I not? I would guess that anyone who personally knows an astronaut living on the ISS would feel closer to being in space. The personal connection means you are paying close attention to everything the astronaut is doing, and following the mission very closely.
The fact that I am sharing so much of what Luca is doing as part of my role as his Earth Liaison also helps me feel closer to being in space, because I am sharing with so many people and they in turn offer me support everyday towards my goals. I watch Luca and can imagine the day when it’s my turn to go into space. It’s been an incredible experience to get to be part of his mission.
Finally, we had clear skies for a terrific Virtual Star Party. Match this with the amazing new high-definition resolution of Google+ Hangouts on Air, and you’ve got a match made in heaven. Astronomers joined us from the West Coast, the East Coast and even Europe.
But the technology gods wouldn’t let these gifts go unpunished. Almost every one of the astronomers wrestled with some kind of technical gremlin.
But if you want to see the Moon and Jupiter in high definition, this was the star party to watch.
We have a Virtual Star Party every Sunday night on Google+ when it gets dark on the West Coast. Currently, that’s about 8 pm Pacific / 11 pm Eastern. We’ll broadcast a live view of the night sky from multiple telescopes across the world.
Subscribe to our YouTube Channel to get notified when there are new parties going live.
