Time for another detailed look at a constellation; one of the most fascinating in the sky, but hidden to most of the northern hemisphere: Carina. Home to one of the most likely supernova candidates we know of: Eta Carinae. Let’s talk just about this constellation, how to find it, and what you can discover in and around it.
You can watch us record Astronomy Cast live every Monday at 12:00 pm PDT (3:00 pm EDT, 2000 GMT). Make sure you circle Fraser on Google+ to see it show up in the feed. You can also see it live over on our YouTube channel.
If you’d like to be notified of all our live events, sign up for our notification email at Cosmoquest. You can check out our calendar here.
I organized three astronomers on Wednesday, but only one had clear skies: Stuart Forman. We got some great views of Jupiter, and attempted a few other objectives. We were joined by Phil Plait, Gary Gonella and Mike Phillips, to showcase some of the recent photos they’ve taken and to talk about gear.
If you want to participate in a future Hangout, please let me know. You just need the ability to display live images or video from your telescope into your computer. From there we can get your view into the Hangout. If you want to participate, please drop me an email at [email protected]. And if you want to be notified when future virtual star parties are happening, circle me on Google+.
[/caption] Here’s a photograph of Jupiter that Stuart created based on the video he captured during the hangout. He stacked the video frames together using a software tool called Registax.
This is going to be one of the “how we know what we know” kind of shows. How do scientist determine the age of things? How do we know the age of everything from stone tools, to the age of the Earth, to the age of the very Universe.
You can watch us record Astronomy Cast live every Monday at 12:00 pm PDT (3:00 pm EDT, 2000 GMT). Make sure you circle Fraser on Google+ to see it show up in the feed. You can also see it live over on our YouTube channel.
If you’d like to be notified of all our live events, sign up for our notification email at Cosmoquest. You can check out our calendar here.
For those of you following me on Google+, you know that I’ve been hosting virtual star parties with Phil Plait and Pamela Gay. We’ve teamed up with astronomer Mike Phillips who has been livestreaming his telescopes into a Google+ Hangout and then broadcasting it live so everyone can watch. So, it’s sort of like looking through an amazing telescope, but with color commentary from us at the same time.
It’s been an amazing experience so far, but I know it can be even better. I need to find more astronomers able to livestream the view from their telescopes into a webcam and then into a Google+ Hangout. I’d like to have multiple telescopes going at the same time, with different views of the skies. Some focused on planets, others at deep sky objects.
And it doesn’t have to be big telescopes. There are beautiful objects in the sky, like open clusters, which look better with a wider field of view.
So, if you’re interested in participating, you’ll need to have a way to get the view from your telescope, into a webcam, and then use that webcam to join a Google+ Hangout. If you can do that, drop me an email at [email protected] and we’ll run some tests.
Here are two previous nights of experiments that we’ve done so far.
This was the first weekly space hangout, run as a Hangout on Air in Google+. On the agenda: NASA’s GRAIL Mission, the return of Phobos-Grunt, the Quadrantid meteor shower, 2012 nonsense and teleporting Obama to Mars. We were joined by Nancy Atkinson, Alan Boyle, Fraser Cain, Pamela Gay, Nicole Gugliucci, Ian O’Neill, Phil Plait, and Jon Voisey.
I apologize for the low quality of audio and video, we’re working out ways to make this all better, but I hope you enjoy the discussion.
This article was originally written in 2008, but we created a cool video to go along with it yesterday
Let’s find out why Pluto is no longer considered a planet.
Pluto was first discovered in 1930 by Clyde W. Tombaugh at the Lowell Observatory in Flagstaff Arizona. Astronomers had long predicted that there would be a ninth planet in the Solar System, which they called Planet X. Only 22 at the time, Tombaugh was given the laborious task of comparing photographic plates. These were two images of a region of the sky, taken two weeks apart. Any moving object, like an asteroid, comet or planet, would appear to jump from one photograph to the next.
After a year of observations, Tombaugh finally discovered an object in the right orbit, and declared that he had discovered Planet X. Because they had discovered it, the Lowell team were allowed to name it. They settled on Pluto, a name suggested by an 11-year old school girl in Oxford, England (no, it wasn’t named after the Disney character, but the Roman god of the underworld).
The Solar System now had 9 planets.
Astronomers weren’t sure about Pluto’s mass until the discovery of its largest Moon, Charon, in 1978. And by knowing its mass (0.0021 Earths), they could more accurately gauge its size. The most accurate measurement currently gives the size of Pluto at 2,400 km (1,500 miles) across. Although this is small, Mercury is only 4,880 km (3,032 miles) across. Pluto is tiny, but it was considered larger than anything else past the orbit of Neptune.
Over the last few decades, powerful new ground and space-based observatories have completely changed previous understanding of the outer Solar System. Instead of being the only planet in its region, like the rest of the Solar System, Pluto and its moons are now known to be just a large example of a collection of objects called the Kuiper Belt. This region extends from the orbit of Neptune out to 55 astronomical units (55 times the distance of the Earth to the Sun).
Astronomers estimate that there are at least 70,000 icy objects, with the same composition as Pluto, that measure 100 km across or more in the Kuiper Belt. And according to the new rules, Pluto is not a planet. It’s just another Kuiper Belt object.
Here’s the problem. Astronomers had been turning up larger and larger objects in the Kuiper Belt. 2005 FY9, discovered by Caltech astronomer Mike Brown and his team is only a little smaller than Pluto. And there are several other Kuiper Belt objects in that same classification.
Astronomers realized that it was only a matter of time before an object larger than Pluto was discovered in the Kuiper Belt.
And in 2005, Mike Brown and his team dropped the bombshell. They had discovered an object, further out than the orbit of Pluto that was probably the same size, or even larger. Officially named 2003 UB313, the object was later designated as Eris. Since its discovery, astronomers have determined that Eris’ size is approximately 2,600 km (1,600 miles) across. It also has approximately 25% more mass than Pluto.
With Eris being larger, made of the same ice/rock mixture, and more massive than Pluto, the concept that we have nine planets in the Solar System began to fall apart. What is Eris, planet or Kuiper Belt Object; what is Pluto, for that matter? Astronomers decided they would make a final decision about the definition of a planet at the XXVIth General Assembly of the International Astronomical Union, which was held from August 14 to August 25, 2006 in Prague, Czech Republic.
Astronomers from the association were given the opportunity to vote on the definition of planets. One version of the definition would have actually boosted the number of planets to 12; Pluto was still a planet, and so were Eris and even Ceres, which had been thought of as the largest asteroid. A different proposal kept the total at 9, defining the planets as just the familiar ones we know without any scientific rationale, and a third would drop the number of planets down to 8, and Pluto would be out of the planet club. But, then… what is Pluto?
In the end, astronomers voted for the controversial decision of demoting Pluto (and Eris) down to the newly created classification of “dwarf planet”.
Is Pluto a planet? Does it qualify? For an object to be a planet, it needs to meet these three requirements defined by the IAU:
It needs to be in orbit around the Sun – Yes, so maybe Pluto is a planet.
It needs to have enough gravity to pull itself into a spherical shape – Pluto…check
It needs to have “cleared the neighborhood” of its orbit – Uh oh. Here’s the rule breaker. According to this, Pluto is not a planet.
What does “cleared its neighborhood” mean? As planets form, they become the dominant gravitational body in their orbit in the Solar System. As they interact with other, smaller objects, they either consume them, or sling them away with their gravity. Pluto is only 0.07 times the mass of the other objects in its orbit. The Earth, in comparison, has 1.7 million times the mass of the other objects in its orbit.
Any object that doesn’t meet this 3rd criteria is considered a dwarf planet. And so, Pluto is a dwarf planet. There are still many objects with similar size and mass to Pluto jostling around in its orbit. And until Pluto crashes into many of them and gains mass, it will remain a dwarf planet. Eris suffers from the same problem.
It’s not impossible to imagine a future, though, where astronomers discover a large enough object in the distant Solar System that could qualify for planethood status. Then our Solar System would have 9 planets again.
Even though Pluto is a dwarf planet, and no longer officially a planet, it’ll still be a fascinating target for study. And that’s why NASA has sent their New Horizons spacecraft off to visit it. New Horizons will reach Pluto in July 2015, and capture the first close-up images of the (dwarf) planet’s surface.
Space enthusiasts will marvel at the beauty and remoteness of Pluto, and the painful deplaneting memories will fade. We’ll just be able to appreciate it as Pluto, and not worry how to categorize it. At least now you know why Pluto was demoted.
Thanks to the power of Google+ Hangouts on Air, we’re now able broadcast live video hangouts with a worldwide audience.
We’re planning to run these Hangouts on a regular schedule, live on Google+. We’ll post a link when the Hangout is about to begin, but if you want to get notified, make sure you circle Fraser Cain on Google+ – then you’ll see the Hangout in your stream when it has begun.
You don’t need to be a member of Google+ to watch them, we’ll post a public link when we’re getting started here, on Google+, Twitter and Facebook. We’ll post the completed videos to Youtube after the fact.
I’ve put a countdown timer over on the right-hand side of Universe Today, so you can see time until the next video hangout.
We currently have two weekly “shows” planned, with more to come:
Weekly Space Roundup – Thursdays at 10:00am PST
Once a week, we’ll pull together the combined space reporting power of Universe Today, Bad Astronomy, MSNBC, Planetary Society, Discovery.com and other space news outlets to give you an overview of what’s going on… out there.
We’ll update you on the week’s big space news stories and provide our expert analysis. Since this is live, you’ll be able to participate in the conversation, asking questions to our team.
Astronomy Cast Live – Time to be determined
Watch Fraser Cain and Dr. Pamela Gay record Astronomy Cast as a live Google+ Hangout. Then join us after the show for an actual hangout. We’ll chat with fans about the topic we discussed and answer general space and astronomy questions.
It’s been one more day since Colin Legg posted his previous amazing photos and videos of Comet Lovejoy. This new version is even better, especially with it reflecting off the water.
Here’s what Colin had to say about it on IceinSpace:
Had another lovely view of the comet last night wandering the shore of the Estuary. It’s quite unique down there. The Perth and Mandurah sky domes light up the northern half of the sky, while the east and south east are pitch black (except for a couple of small towns). The north glow is enough to walk by once dark adapted.
Anyway, while wandering I came across a small embayment with still water and nice reflections of the comet. Used the same settings as last night to get the attached shot.
I’ve finally figured out what to do with all the browser tabs that I have open, but never get around to using: Tumblr. Our new Tumblr blog is a slush pile of links, photos and videos that we just don’t have the time or energy to incorporate into the main Universe Today blog. I’ll warn you, it could easily be 20+ items a day just dumped in there, so if Universe Today is already overwhelming, that’ll be like drinking from a firehose.
Just to let you know, I’m still wrapping my brain around Tumblr, so if you have any suggestions on how to use it better, I’m all ears.