Category Archives: Solar System

Tiny satellites poised to make big contributions to essential science


Tiny satellites, some smaller than a shoe box, are currently orbiting around 200 miles above Earth, collecting data about our planet and the universe. It’s not just their small stature but also their accompanying smaller cost that sets them apart from the bigger commercial satellites that beam phone calls and GPS signals around the world, for instance. These SmallSats are poised to change the way we do science from space. Their cheaper price tag means we can launch more of them, allowing for constellations of simultaneous measurements from different viewing locations multiple times a day – a bounty of data which would be cost-prohibitive with traditional, larger platforms.

Called SmallSats, these devices can range from the size of large kitchen refrigerators down to the size of golf balls. Nanosatellites are on that smaller end of the spectrum, weighing between one and 10 kilograms and averaging the size of a loaf of bread.

Starting in 1999, professors from Stanford and California Polytechnic universities established a standard for nanosatellites. They devised a modular system, with nominal units (1U cubes) of 10x10x10 centimeters and 1kg weight. CubeSats grow in size by the agglomeration of these units – 1.5U, 2U, 3U, 6U and so on. Since CubeSats can be built with commercial off-the-shelf parts, their development made space exploration accessible to many people and organizations, especially students, colleges and universities. Increased access also allowed various countries – including Colombia, Poland, Estonia, Hungary, Romania and Pakistan – to launch CubeSats as their first satellites and pioneer their space exploration programs.

Initial CubeSats were designed as educational tools and technological proofs-of-concept, demonstrating their ability to fly and perform needed operations in the harsh space environment. Like all space explorers, they have to contend with vacuum conditions, cosmic radiation, wide temperature swings, high speed, atomic oxygen and more. With almost 500 launches to date, they’ve also raised concerns about the increasing amount of “space junk” orbiting Earth, especially as they come almost within reach for hobbyists. But as the capabilities of these nanosatellites increase and their possible contributions grow, they’ve earned their own place in space.

From proof of concept to science applications

When thinking about artificial satellites, we have to make a distinction between the spacecraft itself (often called the “satellite bus”) and the payload (usually a scientific instrument, cameras or active components with very specific functions). Typically, the size of a spacecraft determines how much it can carry and operate as a science payload. As technology improves, small spacecraft become more and more capable of supporting more and more sophisticated instruments.

These advanced nanosatellite payloads mean SmallSats have grown up and can now help increase our knowledge about Earth and the universe. This revolution is well underway; many governmental organizations, private companies and foundations are investing in the design of CubeSat buses and payloads that aim to answer specific science questions, covering a broad range of sciences including weather and climate on Earth, space weather and cosmic rays, planetary exploration and much more. They can also act as pathfinders for bigger and more expensive satellite missions that will address these questions.

I’m leading a team here at the University of Maryland, Baltimore County that’s collaborating on a science-focused CubeSat spacecraft. Our Hyper Angular Rainbow Polarimeter (HARP) payload is designed to observe interactions between clouds and aerosols – small particles such as pollution, dust, sea salt or pollen, suspended in Earth’s atmosphere. HARP is poised to be the first U.S. imaging polarimeter in space. It’s an example of the kind of advanced scientific instrument it wouldn’t have been possible to cram onto a tiny CubeSat in their early days.

HARP spacecraft and payload at different stages of development.
Spacecraft: SDL, Payload:UMBC, CC BY-ND

Funded by NASA’s Earth Science Technology Office, HARP will ride on the CubeSat spacecraft developed by Utah State University’s Space Dynamics Lab. Breaking the tradition of using consumer off-the-shelf parts for CubeSat payloads, the HARP team has taken a different approach. We’ve optimized our instrument with custom-designed and custom-fabricated parts specialized to perform the delicate multi-angle, multi-spectral polarization measurements required by HARP’s science objectives.

HARP is currently scheduled for launch in June 2017 to the International Space Station. Shortly thereafter it will be released and become a fully autonomous, data-collecting satellite.

SmallSats – big science

HARP is designed to see how aerosols interact with the water droplets and ice particles that make up clouds. Aerosols and clouds are deeply connected in Earth’s atmosphere – it’s aerosol particles that seed cloud droplets and allow them to grow into clouds that eventually drop their precipitation.

Pollution particles lead to precipitation changes.
Martins, UMBC, CC BY-ND

This interdependence implies that modifying the amount and type of particles in the atmosphere, via air pollution, will affect the type, size and lifetime of clouds, as well as when precipitation begins. These processes will affect Earth’s global water cycle, energy balance and climate.

When sunlight interacts with aerosol particles or cloud droplets in the atmosphere, it scatters in different directions depending on the size, shape and composition of what it encountered. HARP will measure the scattered light that can be seen from space. We’ll be able to make inferences about amounts of aerosols and sizes of droplets in the atmosphere, and compare clean clouds to polluted clouds.

In principle, the HARP instrument would have the ability to collect data daily, covering the whole globe; despite its mini size it would be gathering huge amounts of data for Earth observation. This type of capability is unprecedented in a tiny satellite and points to the future of cheaper, faster-to-deploy pathfinder precursors to bigger and more complex missions.

HARP is one of several programs currently underway that harness the advantages of CubeSats for science data collection. NASA, universities and other institutions are exploring new earth sciences technology, Earth’s radiative cycle, Earth’s microwave emission, ice clouds and many other science and engineering challenges. Most recently MIT has been funded to launch a constellation of 12 CubeSats called TROPICS to study precipitation and storm intensity in Earth’s atmosphere.

For now, size still matters

But the nature of CubeSats still restricts the science they can do. Limitations in power, storage and, most importantly, ability to transmit the information back to Earth impede our ability to continuously run our HARP instrument within a CubeSat platform.

So as another part of our effort, we’ll be observing how HARP does as it makes its scientific observations. Here at UMBC we’ve created the Center for Earth and Space Studies to study how well small satellites do at answering science questions regarding Earth systems and space. This is where HARP’s raw data will be converted and interpreted. Beyond answering questions about cloud/aerosol interactions, the next goal is to determine how to best use SmallSats and other technologies for Earth and space science applications. Seeing what works and what doesn’t will help inform larger space missions and future operations.

The SmallSat revolution, boosted by popular access to space via CubeSats, is now rushing toward the next revolution. The next generation of nanosatellite payloads will advance the frontiers of science. They may never supersede the need for bigger and more powerful satellites, but NanoSats will continue to expand their own role in the ongoing race to explore Earth and the universe.

The Conversation

J. Vanderlei Martins, Professor of Physics, University of Maryland, Baltimore County

This article was originally published on The Conversation. Read the original article.

Do no harm to life on Mars? Ethical limits of the ‘Prime Directive’


NASA’s chief scientist recently announced that “…we’re going to have strong indications of life beyond Earth within a decade, and I think we’re going to have definitive evidence within 20 to 30 years.” Such a discovery would clearly rank as one of the most important in human history and immediately open up a series of complex social and moral questions. One of the most profound concerns is about the moral status of extraterrestrial life forms. Since humanities scholars are only just now beginning to think critically about these kinds of post-contact questions, naïve positions are common.

Take Martian life: we don’t know if there is life on Mars, but if it exists, it’s almost certainly microbial and clinging to a precarious existence in subsurface aquifers. It may or may not represent an independent origin – life could have emerged first on Mars and been exported to Earth. But whatever its exact status, the prospect of life on Mars has tempted some scientists to venture out onto moral limbs. Of particular interest is a position I label “Mariomania.”

Should we quarantine Mars?

Mariomania can be traced back to Carl Sagan, who famously proclaimed

If there is life on Mars, I believe we should do nothing with Mars. Mars then belongs to the Martians, even if the Martians are only microbes.

Chris McKay, one of NASA’s foremost Mars experts, goes even further to argue that we have an obligation to actively assist Martian life, so that it does not only survives, but flourishes:

…Martian life has rights. It has the right to continue its existence even if its extinction would benefit the biota of Earth. Furthermore, its rights confer upon us the obligation to assist it in obtaining global diversity and stability.

To many people, this position seems noble because it calls for human sacrifice in the service of a moral ideal. But in reality, the Mariomaniac position is far too sweeping to be defensible on either practical or moral grounds.

Streaks down Martian mountains are evidence of liquid water running downhill – and hint at the possibility of life on the planet.
NASA/JPL/University of Arizona, CC BY

A moral hierarchy: Earthlings before Martians?

Suppose in the future we find that:

  1. There is (only) microbial life on Mars.
  2. We have long studied this life, answering our most pressing scientific questions.
  3. It has become feasible to intervene on Mars in some way (for instance, by terraforming or strip mining) that would significantly harm or even destroy the microbes, but would also be of major benefit to humanity.

Mariomaniacs would no doubt rally in opposition to any such intervention under their “Mars for the Martians” banners. From a purely practical point of view, this probably means that we should not explore Mars at all, since it is not possible to do so without a real risk of contamination.

Beyond practicality, a theoretical argument can be made that opposition to intervention might itself be immoral:

  • Humans beings have an especially high (if not necessarily unique) moral value and thus we have an unambiguous obligation to serve human interests.
  • It is unclear if Martian microbes have moral value at all (at least independent of their usefulness to people). Even if they do, it’s certainly much less than that of human beings.
  • Interventions on Mars could be of enormous benefit to humankind (for instance, creating a “second Earth”).
  • Therefore: we should of course seek compromise where possible, but to the extent that we are forced to choose whose interests to maximize, we are morally obliged to err on the side of humans.

Obviously, there are a great many subtleties I don’t consider here. For example, many ethicists question whether human beings always have higher moral value than other life forms. Animal rights activists argue that we should accord real moral value to other animals because, like human beings, they possess morally relevant characteristics (for instance, the ability to feel pleasure and pain). But very few thoughtful commentators would conclude that, if we are forced to choose between saving an animal and saving a human, we should flip a coin.

Simplistic claims of moral equality are another example of overgeneralizing a moral principle for rhetorical effect. Whatever one thinks about animal rights, the idea that the moral status of humans should trump that of microbes is about as close to a slam dunk as it gets in moral theory.

On the other hand, we need to be careful since my argument merely establishes that there can be excellent moral reasons for overriding the “interests” of Martian microbes in some circumstances. There will always be those who want to use this kind of reasoning to justify all manner of human-serving but immoral actions. The argument I outline does not establish that anyone should be allowed to do anything they want to Mars for any reason. At the very least, Martian microbes would be of immense value to human beings: for example, as an object of scientific study. Thus, we should enforce a strong precautionary principle in our initial dealings with Mars (as a recent debate over planetary protection policies illustrates).

For every complex question, there’s a simple, incorrect answer

Mariomania seems to be the latest example of the idea, common among undergraduates in their first ethics class, that morality is all about establishing highly general rules that admit no exception. But such naïve versions of moral ideals don’t long survive contact with the real world.

By way of example, take the “Prime Directive” from TV’s “Star Trek”:

…no Star Fleet personnel may interfere with the normal and healthy development of alien life and culture…Star Fleet personnel may not violate this Prime Directive, even to save their lives and/or their ship…This directive takes precedence over any and all other considerations, and carries with it the highest moral obligation.

Hollywood’s version of moral obligation can be a starting point for our real-world ethical discussion.

As every good trekkie knows, Federation crew members talk about the importance of obeying the prime directive almost as often as they violate it. Here, art reflects reality, since it’s simply not possible to make a one-size-fits-all rule that identifies the right course of action in every morally complex situation. As a result, Federation crews are constantly forced to choose between unpalatable options. On the one hand, they can obey the directive even when it leads to clearly immoral consequences, as when the Enterprise refuses to cure a plague devastating a planet. On the other hand, they can generate ad hoc reasons to ignore the rule, as when Captain Kirk decides that destroying a supercomputer running an alien society doesn’t violate the spirit of the directive.

Of course, we shouldn’t take Hollywood as a perfect guide to policy. The Prime Directive is merely a familiar example of the universal tension between highly general moral ideals and real-world applications. We will increasingly see the kinds of problems such tension creates in real life as technology opens up vistas beyond Earth for exploration and exploitation. If we insist on declaring unrealistic moral ideals in our guiding documents, we should not be surprised when decision makers are forced to find ways around them. For example, the U.S. Congress’ recent move to allow asteroid mining can be seen as flying in the face of the “collective good of mankind” ideals expressed in the Outer Space Treaty signed by all space-faring nations.

The solution is to do the hard work of formulating the right principles, at the right level of generality, before circumstances render moral debate irrelevant. This requires grappling with the complex trade-offs and hard choices in an intellectually honest fashion, while refusing the temptation to put forward soothing but impractical moral platitudes. We must therefore foster thoughtful exchanges among people with very different conceptions of the moral good in order to find common ground. It’s time for that conversation to begin in earnest.

The Conversation

Kelly C. Smith, Associate Professor of Philosophy & Biological Sciences, Clemson University

This article was originally published on The Conversation. Read the original article.

Kepler Confirms 1,284 Exoplanets Outside Solar System


A study published yesterday in the Astrophysical Journal by a group of researchers confirms an additional 1,284 exoplanets have been spotted by Kepler, NASA’s planet-hunting spacecraft. That brings the total number of verified exoplanets from Kepler to more than 2,000 — more than doubling the amount spotted by the spacecraft.

“We have more than doubled the number of known exoplanets smaller than the size of Neptune,” Tim Morton, an associate research scholar at Princeton University.

For the complete study, visit The Astrophysical Journal.

Astrobiologists Use Biosignature Gases To Search For Aliens


Professor Sara Seager of Massachusetts Institute of Technology says her team of scientists is looking for biosignatures from gases emitted by alien life forms on habitable extrasolar planets. Many of these gases could be detected remotely by telescopes, but could end up having quite different compositions from those in the atmosphere of our planet.

Prof. Seager and her colleagues explained,

“Thousands of exoplanets are known to orbit nearby stars. Plans for the next generation of space-based and ground-based telescopes are fueling the anticipation that a precious few habitable planets can be identified in the coming decade. Even more highly anticipated is the chance to find signs of life on these habitable planets by way of biosignature gases.”

Seager’s team proposes in their paper published online in the journal Astrobiology that all stable and potential volatile molecules should be considered as possible biosignature gases, laying the groundwork for identifying such gases by conducting a massive search for molecules with six or fewer non-hydrogen atoms in order to maximize their chances of recognizing biosignature gases. They say they promote the concept that “all stable and potentially volatile molecules should initially be considered as viable biosignature gases.”

The scientists created a list of about 14,000 molecules that contain up to 6 non-H atoms. About 2,500 of these are CNOPSH (C – carbon, N – nitrogen, O – oxygen, P – phosphorus, S – sulfur, and H – hydrogen) compounds.

This means that instead of the costly and controversial method of netting strange creatures from the bottom of the sea, these scientists have decided to search and find thousands of curious, potentially biogenic gas molecules.

Mars and Earth are getting closer together


On May 30, our cold, red sandy neighbor outside Earth’s orbit is getting very close to us, at least for a short duration of time.

Scientists say Mars will be closer to Earth than it’s been since the past eleven years. At about 46.8 million miles away, it’s still a rather distant journey away, but the planet can typically be about 250 million miles away.

According to NASA, from May 18th until June 3rd, the great red planet will be bigger, brighter and hopefully more visible, weather permitting.

Skywatchers should expect to see a reddish star in the mornings at dawn or slightly before, if you are in the UK. United States watchers should look for it around midnight.

For a better view, look up your local astronomy club where members are likely to have powerful telescopes. If you’re looking for a telescope yourself, check out the Celestron C9.25 and get ready for some mindblowing astronomy at home.

Disturbing Mars Weather Concerns NASA About Affects of Sun Spots On Earth


Recently, NASA revealed about some sensitive details concerning massive storms that destroyed Mars’ atmosphere. They went on to enquire how ready are we to accept and combat such a “high impact event.” This announcement comes after NASA’s Mars Atmosphere and Volatile Evolution (MAVEN) spacecraft, which spotted how the massive storm that, stripped away the planet’s atmosphere.

Commenting on this activity, Joe Grebowsky, MAVEN’s project scientist said that solar storms and wind corrosion is the key reason for atmospheric loss, and was the main cause for the major changes in the Martian climate.

Post September 2014, MAVEN has pointed out this storm to be the largest. The most important reason why it has become a cause of concern is that such abnormal weather activity can hamper technology-based infrastructures and give rise to many unforeseen accidents.

In 2012, a coronal mass ejection (CME) solar storm just missed a possible collision with earth, due to a sudden eruption in sun. Associating, the current situation, scientists say if such thing is repeated today, the human kind is all set to witness a massive a technological disaster like destroyed satellites, non-functional GPS system.

As far as the costs are concerned Llyod’s pointed out that to prevent from such solar storm will cost somewhere between $600 billion and $2.6 trillion.

Jupiter Known To Have Three Suns In Its Sky


Scientists at the Smithsonian have discovered a giant planet with three suns and which is 685 light years from us.

They said that while one of its Sun is about 40 times more intense than our Sun. It was also believed by the scientists that the KELT-4 system, which is home to a “Hot Jupiter” planet known as KELT-4Ab, is a binary system. However, it was recently discovered that it is instead a binary pair. This finding was possible by the use of two telescopes located in Arizona and South Africa. These two telescopes when combined together are known as Kilodegree Extremely Little Telescope (KELT).

The other two stars, KELT-4B and KELT-4C appeared dimmer, and could be compared to the Earth’s moon.

The star KELT -4A is close to us and it is brighter, making it easier to study. The other two suns are comparatively far away, dimmer and not that large. It takes KELT-4Ab just three days to orbit KELT-4A.The temperature on Hot Jupiter is very high, touching around thousands of degrees Fahrenheit.
KELT-4Ab is the fourth exoplanet, which has been discovered to have three suns. This giant planet is much closer to earth compared to other three planets therefore, it is much more convenient to observe it closely.

Jason Eastman and his colleagues at the Harvard-Smithsonian Center for Astrophysics, plan to further study these stars, and they aim to find out how their gravity pushed KELT-4Ab into such a hot spot.