January 18, 2015 – This is going to be an interesting year for Deep Space exploration. Here are three missions that will achieve significant objectives and milestones in 2015:
Dawn visits Ceres
The asteroid explorer Dawn having visited Vesta back in 2011-12, is quickly approaching the largest object in the Asteroid Belt, the dwarf planet, Ceres. Ceres is the only asteroid that is spherical in shape. It is described by Dawn mission scientists as a complete mystery. Dawn will enter into orbit around Ceres beginning March 6th and will study it for more than a year.
Back in December Dawn took a snapshot of distant Ceres. That highly pixilated image appears below. We have better images from the Hubble Space Telescope but over the next two months we will see Ceres as we have never viewed it before.
Astronomers note that the Texas-sized dwarf planet is largely composed of water ice and on its surface may even have deposits of organic molecules, the building blocks of life. Others suspect a subterranean ocean beneath the icy surface with the potential for life there as well.
New Horizons Reaches Pluto
In July the New Horizons spacecraft will make its closest approach to Pluto. An eight year journey to what was once classified as the ninth planet, but now is relegated to dwarf-planet status, should unlock its mysteries. Pluto, like Ceres, remains a mystery. We know some things about it from spectral observations here on Earth. For example we know it has an atmosphere largely composed of nitrogen. And with an atmosphere we know that Pluto rotates and experiences seasonal changes. Scientists expect to observe the frost cycle, with nitrogen ice sublimating into gas in response to the Sun, as the spacecraft trains its instrumentation for several months both pre and post fly by.
New Horizons will be approaching Pluto at a time when it is moving further from the Sun in its orbital path. At the same time the northern pole of the dwarf planet will be receiving the majority of the Sun’s energy. That should produce some interesting atmospheric dynamics.
From May on we will begin to see pictures of Pluto, Charon and its other four companion moons with clarity far greater than anything seen from Hubble or Earth-based telescopes. And by July the pictures and data we receive should amaze us in the same way the Voyagers did back in the 1970s revealing to us Jupiter, Saturn, Uranus and Neptune.
What Pluto looks like right now from New Horizons can be seen in the image below. Not much to see as of yet but you can detect Charon just to the left.
Akatsuki Visits Venus
The Japanese spacecraft, Akatsuki, will be the first probe from that country to enter orbit around Venus. This should happen sometime in November.
Back in 2010 Akatsuki attempted an orbit-insertion burn on passing Venus but its main engines failed. But the Japanese space agency, JAXA, found a way to use the thrusters on the spacecraft to set up this eventual rendezvous. First they fired them to adjust the spacecraft’s trajectory to create a second rendezvous. With that success they are confident that a second firing of the thrusters will put Akatsuki into a week-long elliptical orbit around Venus.
The orbiter mission will focus on studying the planet’s atmospheric circulation. Instrumentation includes ultraviolet and infrared imaging, lightning detection and a high-speed imager.
eLISA to Study Gravity Waves
The European Space Agency will launch sometime in 2015, the Evolved Laser Interferometer Space Antenna (eLISA). It will be the first combination spacecraft deployed to study gravity waves. Using a laser interferometer a trio of spacecraft, a mother ship and two daughters, hopes to discover the sources of gravity waves and measure them.
First theorized by Albert Einstein, gravity waves made the headlines recently when physicists announced back in March 2014 that they had discovered the first images of ripples in the Universe, gravity waves resulting from the Big Bang, a proof of Einstein’s theory.
Gravity waves are unlike any other type of waves we know. They distort space time by fractionally changing the distance between two objects. eLISA instrumentation will measure tiny changes in distance between objects in free fall within and between the three spacecraft as gravity waves impact them. Spaced 1 million kilometers (620,000 miles) apart in an equilateral triangulation, they will be connected through a high precision interferometer.
Related Posts
How The Rise Of AI Is Shaping The Future Of Business
Why Am I Left-Handed? Blame Tubulin Proteins for This Asymmetric Brain Twist
Conversations About AI: Inoculating Ourselves Against AI Scammers
Conversations With AI: Digital Avatars Give The Speechless The Ability To Speak
Robots in the News: From Tesla Optimus to BMW Figure and More
The Saga of Honeybee Colony Collapse is Being Questioned
Should the U.S. Power Grid Move Underground?
Canada is Becoming a Nuclear Fusion Hotbed
Ceres itself will never be colonized by humans (gravity is too low), but if Ceres actually has the speculated oceans of surface water,it will become the main hub of construction for human space habitats and distant planetary exploration vessels. For all practical purposes, this huge mass of water is already in space with more kinetic energy than it would have were it in Earth orbit.
Sustained human existence requires several factors that are available on Earth, but rare in space: Atmospheric oxygen for respiration, water for biological process, gravity between 0.8 and 1.1 g, and shielding from both radiation and meteorites.
If form is to follow function, practical space habitats or ships for humans must take the form of giant rotating hollow wheels. The rotation supplies the essential artificial gravity. The giant size diminishes Coriolis effects. Only robots working with asteroid materials can produce such structures. One can envision a 1,200 foot diameter space habitat in the asteroid belt supplied with an atmosphere and biotic system derived from the water of Ceres. Millions of tons of “concrete” made from asteroid sand/pebbles and frozen water would provide the shielding. Since propulsion in vacuum depends on expulsion of reaction mass, all space propulsion is limited by
available reaction mass. The water of Ceres could supply inexhaustible reaction mass, so a giant spinning nuclear-powered hollow donut habitat would also be a comfortable interplanetary spaceship that could range anywhere in the solar system and even venture out into and beyond the Ort Cloud. There is no practical limit on how many large wheel ships robots could construct from asteroid belt material. Over several centuries, thousands of these wheel habitat/ships might be assembled by robots in space near Ceres, and eventually all of mankind that wants to leave Earth and livein an artificial space colony would have someplace to go.
These large wheel ships could in principle venture into interstellar space and millions of generations latter approach nearby stars. Then the first order of business would be to locate a water-rich Ceres type body and replenish the ship’s reaction mass and repair shield erosion.
While such an interstellar ship might leave the Sol planetary system with a crew of modern humans and their AI robots, what would eventually arrive at another star some millions of years latter would not likely bear much resemblance to humanity. Such a voyage would amount mostly to a very inefficient form of cosmological panspermia.
I’m guessing the first of many asteroid belt wheel-ships to follow will begin construction in the late 2040s.
I have tweeted your reply to this posting. Allen, I would love if you could turn this into a guest blog entry on the site if you are up to it.