One of the most important questions our species has tackled is the origin of life on Earth. If we can figure out the conditions and catalyst for the beginning of life, we can look elsewhere in the universe for those same conditions, and zero in on the potential for finding extraterrestrial life. We know the universe is old enough for the painstakingly slow evolutionary process, but what started it? In the famous 1952 Miller-Urey experiment, a flask containing the basic natural elements water (H20), methane (CH4), Ammonia (NH4), and Hydrogen (H2), all present on the early Earth, was subjected to...
Since the arrival of the Dawn spacecraft in March of 2015, we have seen tremendous views of the dwarf planet Ceres. Lying within the asteroid belt, it is revealed to be a frozen world of ice and rock, with many interesting features. None of these features had generated more intrigue than the famous bright spot in the bottom of what is now called the Occator crater. The icy spot has had astronomers guessing for months whether it is a cryovolcano, water ice, frozen carbon dioxide, or something even more strange and rare. As the Dawn spacecraft has moved into a...
The Past: Mars has water, and it used to have a lot more. If modern Mars had the ocean it once had, it would evaporate off into space quickly because there is no heavy atmosphere to help keep it pressurized and in liquid form. Mars would have had a thicker atmosphere in addition to it’s magnetic field in order to keep all that water in one place. So where did the atmosphere go? And if there was such a thick atmosphere, how does it account for the fingerprint of excess Carbon-13 and a lack of Carbon-12 found on the red planet...
A few weeks back, the Philae lander woke up and began transmitting the coveted science data it had been holding on to for the better part of 2015, waiting for the Sun to shine bright enough to wake it from its deep slumber. As soon as it was able, it transmitted data back to the Rosetta orbiter, which then sent it on its long journey back home to Earth. Now that a few weeks have passed, we can finally see what the first science from the surface of 67P looks like, and determine its true fate. We can clearly see a...
The Rosetta orbiter, currently studying comet 67P/Churyumov-Gerasimenko as it orbits the Sun, has been watching how the comet has changed as it moves toward its perihelion (point of closest approach to the Sun) in August of 2015. As the comet heats up from the increasing intensity of the Sun’s rays, it releases surface gases and dust into what eventually becomes the atmosphere-like coma surrounding the comet. As the comet moves the material produces the visible tail that we usually associate with a comet. With 67P specifically, Rosetta has recently made a surprising discovery: That the water and carbon dioxide streaming...
By now, if you keep up with Astronomy news even a little bit, you’ve heard of the strange white spot on the surface of Ceres, within a large crater in the dwarf planet’s northern hemisphere. As the science mission of the Dawn spacecraft continues, we are starting to see new images of the surface in unprecedented detail, and finally we have a closer view of the mystery spot. Is the new series of images enough to determine its origin? See for yourself. The only thing clear from these new images is that what once appeared to be a single or...
As the Dawn Spacecraft readies for orbit insertion only a week from now, the images coming in are getting sharper and sharper. Once the craft is fully in orbit its first task will be to map the surface of the planet in high definition. Even on the last few weeks of the journey to Ceres, we have seen increasingly clear images, and have already started asking ‘What the heck is that?’ This week’s ‘what the heck are we looking at?’ involves this apparent double bright spot on Ceres, imaged on February 19th from a distance of 46,000 Km, about an...
Venus is the most hellish place I know of in the Solar System, and maybe even the broader Universe. Even though Venus looks pretty harmless and is named for the Roman goddess of Love, beneath the soft looking clouds lies sulphuric acid rainfall, 450 degree surface temperatures, and crushing pressure 90 times the atmospheric pressure of Earth at sea level. How do we get the surface picture of Venus above? NASA’s Magellan probe in 1994 finished mapping the surface by looking at Radio wavelengths emitted by the planet and using radar to bounce waves off the surface to measure features....
