Showing posts with label Ceres. Show all posts
Showing posts with label Ceres. Show all posts

Monday, May 9, 2011

Life on Ceres

I like to look at my stats and see what people are searching for when they come across my blog. A while ago I got a hit from a search for 'Life on Ceres,' and ever since then I have been considering writing a post about it. So this is for you, person out there looking for information about life on Ceres, and hopefully other readers will enjoy this as well.


I had previously glossed over Ceres in my Asteroids Astro-Lesson. Ceres is the largest object in the asteroid belt, and recently got reclassified to a dwarf planet. It is also the smallest known dwarf planet, Pluto (the former smallest planet) is 14 times more massive. And yet Ceres comprises about 25% of the asteroid belt's mass. Ceres is large enough to shape itself into a sphere, at about 580 miles (930 kilometers) across.

But aside from being a unique and astounding body in the asteroid belt, Ceres may have large amounts of water buried under the crust. Astronomers have suggested this because the ex-asteroid's density is less then that of the Earth's crust, because the surface bears spectral evidence of water-bearing minerals. If 25% of Ceres was composed of water, it would have more than all the fresh water on Earth.

The possible internal structure for Ceres. (NASA)

The majority of the water would be ice, forming a mantle around a rocky inner core, with a dusty crust above. It is currently unknown if liquid water exists on Ceres, but a few astronomers suspect there could be oceans. These oceans could be heated by hydrothermal vents and provide a thriving ecology of basic lifeforms.

The problem with this scenario though, is that it is not clear what would keep the proposed oceans in a liquid state. There is no significant tectonic activity (nor enough mass to sustain a long-term molten core) and no significant tidal friction (like with Europa orbiting Jupiter). Although the idea has some merit for consideration, and provides interesting research. We will have to wait until the Dawn spacecraft arrives in 2015 for any definitive answers.

Now, this is where the idea gets a little fun and funky. Supposing Ceres did have a molten core when it and the rest of the Solar System were young, it could have heated an ocean and produced early lifeforms. Well, we know that early Ceres had an active period of bombardment, where meteorites and smaller asteroids impacted and knocked small chunks off. In fact, there is an entire family of asteroids designated C-type because they share similarities with Ceres and many are thought to originate from there. They also happen to be the most common type of asteroid, carbonaceous asteroids.


What I am getting at here is the idea of panspermia, that life in the Universe can start at one place and be transported to others by meteoroids, asteroids, and comets. Ceres has a low escape velocity, so it is not improbably that any early life forms would be kicked off by an impact. That life could have then been transported to Earth, and we could be the descendants.

This is just conjecture. I should put that as a warning, that there is no solid evidence for this hypothesis, but it exists and it is a tantalizing one to discuss. And it is not wholly impossible, but we really don't know. At least not until we find some body whizzing around the Solar System carrying archaic lifeforms most likely in a dormant state. And even if a lifeform made it to Earth, there's no certainty that it survived, life could have already arisen on Earth and devastated the visitor.

The Earth seems to have perfect conditions for life, and must have had sufficient starting conditions. If life was so well at taking hold here, we could it not be formed here in the first place? Then again, maybe there weren't sufficient conditions to start life. Scientifically speaking, there is no clear definition of what caused life to spark into existence on Earth, and panspermia has been a way to address that. But it still neglects the fact that life would have had to have started somewhere at some point in time.


As we get better at understanding biology and Earth's history, this answer is getting clearer. It is now possible, with the right chemical mixtures that relates to the known early atmosphere of the Earth, to generate complex amino acids and other biological components. I suspect we are really only a few years short of understanding the sparking event that unleashed life on Earth, or at least the origin of life somewhere in the Universe if it was brought to Earth.


Tuesday, April 26, 2011

Astro-Lesson: Asteroids

So the poll was a tie between the Sun and asteroids. I just picked asteroids, and will do the Sun next week while I think of new topics to populate the poll. Honestly, I might go back to the question and answer format I did when I started the blog, at least temporarily. It's funny though, even though I've been wanting to do the asteroids, I am having some problems on thinking of how to get started...

Artist Concept of the Asteroid Belt. (NASA)
Astronomers have been studying asteroids for a couple hundred years. The first asteroid discovered was Ceres, in 1801. Now there are over a million asteroids that have been observed flinging like crazy throughout our Solar System. It is estimated nearly 2 million asteroids 1 km or larger reside in the asteroid belt, a region of space between Mars and Jupiter, but other significant populations include Near-Earth asteroids (NEAs) and Trojans. They are left over remnant from the early Solar System and can say a lot about the composition of those early conditions.

The asteroid belt is incredibly diffuse, where spacecraft can fly through it without worry of hitting anything, unlike what may be portrayed in science fiction. The asteroid belt also isn't likely to have been a planet that never formed or got ripped apart by Jupiter, the total mass off the asteroid belt is less than that of our Moon. Collisions do happen between asteroids though, spawning more smaller asteroids, and because they share orbital characteristics and make up, they are grouped into "families." The characteristics of each family also casts doubt on the possibility of planet formation.

Vesta (left) and Ceres (middle) compared to the Moon (right). (NASA)
The largest and  most massive object in the asteroid belt is the dwarf planet Ceres. For a half a century after it was discovered, it was considered a planet, along with the asteroids Pallas (discovered 1802), Juno (1804), and Vesta (1807). No new asteroid would be discovered for nearly 40 years. With the discovery of more, the term planet fell out of favor (no vote or decision was needed like in the case of dwarf planets.) Asteroid had been used interchangeably with planet to describe these objects from the beginning, and took over to describe these "minor planets." Asteroid literally means star-like, because of the objects initial appearance in telescopes was like that of a star, except they moved like planets.

The Asteroid Belt (white) and Jupiter's Trojans (green). (Wikipedia)

Trojans are populations of asteroids that share an orbit with a larger planet or moon, but do not collide with it because they orbit in one of the two Lagrangian points of stability, L4 and L5, which lie 60° ahead of and behind the larger body. The largest group of these are the Jupiter Trojans, which, though few are currently known, may be as numerous as the asteroid belt. Trojans are also found around Neptune and Mars.

Near-Earth asteroids are ones with orbits that pass close to the Earth's orbit. These asteroids are divided into families: The Atens, usually inside the Earths orbit; The Apollos, which have average orbital radii more than that of the Earth and perihelia less than Earth's aphelion; and the Amors, which have orbits between Earth and Mars and are more like to cross Mars' orbit. As of April 27, 2011, there are 7919 close approach asteroids with 1218 potentially hazardous asteroids. (IAU Minor Planet Center is my source)


From the wonderful Saturday Morning Breakfast Cereal.

Asteroids probably the greatest space-based threat to life on Earth. We know it is a threat from the history of the Earth (see the picture above, part of the reason why I wanted to make this post). Asteroids have had a hand in several mass extinctions, including that of the dinosaurs as evidence from the Yucatan Peninsula crater suggests. It WILL happen again, that factor just being time. I won't even address the whole Asteroid Apophis thing, because it won't hit us. Apophis will get close, even inside the orbits of geosynchronous satellites, but at best, it will be a bright object to watch.

Asteroid Defense Force...

But, that doesn't mean NASA and other space programs aren't doing anything. Aside from the actively searching and tracking potentially hazardous asteroids, scientists are hard at work on designing potential defenses. NASA, ESA, the Planetary Society, and Roscosmos (the Russian Federal Space Agency) are all studying possible deflection methods that include ideas such as nuclear bombardment, kinetic impactors, and gravitational tractors.


There are other reasons to study asteroids as well. Near-Earth asteroids may contain resource deposits that could be mined. This is one of the interesting reasons why I support a manned mission to an asteroid. Though returning to the Moon is a nice idea, asteroids would be easier to mine for resources with the lesser gravity. Those resources could be returned to the Earth to make consumer products, or be manufactured in orbit into necessities and spacecraft for further exploration. Mining them would also reduce ecological destruction on Earth. The key result would be that whichever country did this first would become an economic powerhouse and the sole superpower. But hopefully it would spur competition in other nations and more advance into space, pushing humanity into another golden age.


{Click to Enlarge} Montage of all the asteroid close-ups at this time, to scale. (Planetary Society)
But moving back to the subject, the definition of what exactly an asteroid is is something that has yet to be determined. Technically, based on the 2006 IAU decision that created the dwarf planet classification, everything smaller then a dwarf planet is a 'small solar system body', though the term 'minor planet' is still acceptable. These objects have traditionally been classified as asteroids, comets or meteoroids. 
Meteoroids are the easiest to define, typically anything smaller than ten meters across. The line between asteroids and comets has blurred with further study of the Solar System though. So much so that a new classification, Centaurs, has entered the vernacular. These exhibit both asteroid and comet behaviors, comets have a tail and coma of gas around them, and typically lie inwards of the Kuiper belt and outside the orbit of Jupiter. Kuiper belt objects have also been labelled "objects" to avoid classifying them as either asteroids or comets. This leaves us with a general working definition of asteroids as being minor planets of the inner Solar System, such as the asteroid belt, Jupiter Trojans, and near-Earth objects.

Vesta as seen from the Hubble Space Telescope. (NASA)

There are a few large asteroids in the asteroid belt that need clarification too. Vesta, Pallas, and Hygiea may be classified as dwarf planets when their shapes are better known. My bet is that they will remain asteroids, but for Vesta, a definitive answer will be reached soon. The NASA Dawn mission is orbiting Vesta this year and reach Ceres in 2015. This will provide much needed information on these objects, the largest two in the asteroid belt. (And hopefully I will right an article on both of them soon, as Vesta has become dear to me.)

I took this image of Vesta for my university observational astronomy class.

So there is a basic overlay about asteroids. You can see there are many nuances on this level, and it takes some familiarity to really know about them. There are several different "families" and subgroups, as well as problems with those classifications and how they are determined. But this is all I will leave you with. I hope you learned a lot about asteroids, and you will gain a better understanding on them as more missions are carried out to study them.


Monday, March 21, 2011

Mercurial Monday

I promised to give an overview of my trip to the Applied Physics Lab (APL) at Johns Hopkins University on Saturday, so here we go.

The reason I went to the APL was for the Thrill of Discovery Workshop. Five hours of professional development in space science and engineering supported by NASA's Discovery Program. Though, it ended up being 6 hours as we got there half an hour early and it ran over by half an hour. There was approximately 3 hours in a classroom with hands on learning experiences and other educational tools. Then there was approximately 2 hours of lecture in an auditorium, with Q&A after each speaker. The rest of the time was filled with delays and stuff, I didn't really mind.

So this workshop was happening at 4 different locations across the United States, the Jet Propulsion Lab in California, Johnson Space Center in Houston, TX, the Jackson Middle School Observatory in Minnesota, and of course APL.


Thursday, March 10, 2011

A Message From Ceres

I try to keep this blog relatively clean language wise. But this picture was just to awesome not to share! It also fills some space for a quick post today.
In the future I do plan to talk more about Ceres and Vesta and the other asteroids. They are some of my favorite objects in our solar system.