Rosetta Images Show Comet’s Changing Surface Close Up

Rosetta mission poster showing the deployment of the Philae lander to comet 67P/Churyumov-Gerasimenko.. Credit: ESA/ATG medialab (Rosetta/Philae); ESA/Rosetta/NavCam (comet)

The Rosetta spacecraft learned a great deal during the two years that it spent monitoring Comet 67P/Churyumov-Gerasimenko – from August 6th, 2014 to September 30th, 2016. As the first spacecraft to orbit the nucleus of a comet, Rosetta was the first space probe to directly image the surface of a comet, and observed some fascinating things in the process.

For instance, the probe was able to document some remarkable changes that took place during the mission with its OSIRIS camera. According to a study published today (March. 21st) in Science, these included growing fractures, collapsing cliffs, rolling boulders and moving material on the comet’s surface that buried some features and exhumed others.

These changes were noticed by comparing images from before and after the comet reached perihelion on August 13th, 2015 – the closets point in its orbit around the Sun. Like all comets, it is during this point in 67P/Churyumov-Gerasimenko’s orbit that the surface experiences its highest levels of activity, since perihelion results in greater levels of surface heating, as well as increased tidal stresses.

Images taken by Rosetta’s OSIRIS camera show changes in the surface between 2015 and 2016. Credit: ESA/Rosetta/NAVCAM (top center images); ESA/Rosetta/MPS for OSIRIS Team MPS/UPD/LAM/IAA/SSO/INTA/UPM/DASP/IDA (all others)

Basically, as comets gets closer to the Sun, they experience a combination of in-situ weathering and erosion, sublimation of water-ice, and mechanical stresses arising from an increased spin rate. These processes can be either unique and transient, or they can place over longer periods of time.

As Ramy El-Maarry, a scientist from the Max-Planck Institute for Solar System Research and the lead author of the study, said in an ESA press statement:

“Monitoring the comet continuously as it traversed the inner Solar System gave us an unprecedented insight not only into how comets change when they travel close to the Sun, but also how fast these changes take place.”

For instance, in-situ weathering occurs all over the comet and is the result of heating and cooling cycles that happen on both a daily and a seasonal basis. In the case of 67P/Churyumov-Gerasimenko’s (6.44 Earth years), temperatures range from 180 K (-93 °C; -135 °F) to 230 K (-43 °C; -45 °F) during the course of its orbit. When the comet’s volatile ices warm, they cause consolidated material to weaken, which can cause fragmentation.

Combined with the heating of subsurface ices – which leads to outgassing – this process can result in the sudden collapse of cliff walls. As other photographic evidence that was recently released by the Rosetta science team can attest, this sort of process appears to have taken place in several locations across the comet’s surface.

Images showing a new fracture and boulder movement in Anuket. Credit: ESA/Rosetta/MPS for OSIRIS Team MPS/UPD/LAM/IAA/SSO/INTA/UPM/DASP/ID

Similarly, comets experience increased stress because their spin rates speed up as they gets closer to the Sun. This is believed to be what caused the 500 meter-long (1640 ft) fracture that has been observed in the Anuket region. Originally discovered in August of 2014, this fracture appeared to have grown by 30 meters (~100 ft) when it was observed again in December of 2014.

This same process is believed to be responsible for a new fracture that was identified from OSIRIS images taken in June 2016. This 150-300 meter-long (492 – 984 ft) fracture appears to have formed parallel to the original. In addition, photographs taken in February of 2015 and June of 2016 (shown above) revealed how a 4 meter-wide (13 ft) boulder that was sitting close to the fractures appeared to have moved by about 15 meters (49 ft).

Whether or not the two phenomena are related is unclear. But it is clear that something very similar appears to have taken place in the Khonsu region. In this section of the comet (which corresponds to one of its larger lobes), images taken between May of 2015 and June 2016 (shown below) revealed how a much larger boulder appeared to have moved even farther between the two time periods.

Images showing a moving boulder in the Khonsu region. Credit: ESA/Rosetta/MPS for OSIRIS Team MPS/UPD/LAM/IAA/SSO/INTA/UPM/DASP/IDA

This boulder – which measures some 30 meters (98 ft) across and weighs an estimated 12,800 metric tonnes (~14,100 US tons) – moved a distance of about 140 meters (~460 ft). In this case, outgassing during perihelion is believed to be the culprit. On the one hand, it could have caused the surface material to erode beneath it (thus causing it to roll downslope) or by forcibly pushing it.

For some time, it has been known that comets undergo changes during the course of their orbits. Thanks to the Rosetta mission, scientists have been able to see these processes in action for the first time. Much like all space probes, vital information continues to be discovered long after the Rosetta mission officially came to an end. Who knows what else the probe managed to witness during its historic mission, and which we will be privy to?

Further Reading: ESA

Large Hadron Collider Discovers 5 New Gluelike Particles

A typical LHCb event fully reconstructed. Particles identified as pions, kaon, etc. are shown in different colours. Credit: LHCb collaboration

Since it began its second operational run in 2015, the Large Hadron Collider has been doing some pretty interesting things. For example, starting in 2016, researchers at CERN began using the collide to conduct the Large Hadron Collider beauty experiment (LHCb). This is investigation seeks to determine what it is that took place after the Big Bang so that matter was able to survive and create the Universe that we know today.

In the past few months, the experiment has yielded some impressive results, such as the measurement of a very rare form of particle decay and evidence of a new manifestation of matter-antimatter asymmetry. And most recently, the researchers behind LHCb have announced the discovery of a new system of five particles, all of which were observed in a single analysis.

According to the research paper, which appeared in arXiv on March 14th, 2017, the particles that were detected were excited states of what is known as a “Omega-c-zero” baryon. Like other particles of its kind, the Omega-c-zero is made up of three quarks – two of which are “strange” while the third is a “charm” quark. The existence of this baryon was confirmed in 1994. Since then, researchers at CERN have sought to determine if there were heavier versions.

The LHCb collaboration team. Credit: lhcb-public.web.cern.ch

And now, thanks to the LHCb experiment, it appears that they have found them. The key was to examine the trajectories and the energy left in the detector by particles in their final configuration and trace them back to their original state. Basically, Omega-c-zero particles decay via the strong force into another type of baryon (Xi-c-plus) and then via the weak force into protons, kaons, and pions.

From this, the researchers were able to determine that what they were seeing were Omega-c-zero particles at different energy states (i.e. of different sizes and masses). Expressed in megaelectronvolts (MeV), these particles have masses of 3000, 3050, 3066, 3090 and 3119 MeV, respectively. This discovery was rather unique, since it involved the detection of five higher energy states of a particle at the same time.

This was made possible thanks to the specialized capabilities of the LHCb detector and the large dataset that was accumulated from the first and second runs of the LHC – which ran from 2009 to 2013, and since 2015, respectively. Armed with the right equipment and experience, the researchers were able to identify the particles with an overwhelming level of certainty, ruling out the possibility that it was a statistical fluke in the data.

The discovery is also expected to shed light on some of the deeper mysteries of subatomic particles, like how the three constituent quarks are bound inside a baryon by the “strong force” – i.e. the fundamental force that is responsible for holding the insides of atoms together. Another mystery that this could help resolve in the correlation between different quark states.

The Large Hadron Collider is the world’s largest and most powerful particle accelerator Credit: CERN

As Dr Greig Cowan – a researcher from the University of Edinburgh who works on the LHCb experiment at Cern’s LHC – explained in an interview with the BBC:

“This is a striking discovery that will shed light on how quarks bind together. It may have implications not only to better understand protons and neutrons, but also more exotic multi-quark states, such as pentaquarks and tetraquarks.

The next step will be to determine the quantum numbers of these new particles (the numbers used to identify the properties of a specific particle) as well as determining their theoretical significance. Since it came online, the LHC has been helping to confirm the Standard Model of particle physics, as well as reaching beyond it to explore the greater unknowns of how the Universe came to be, and how the fundamental forces that govern it fit together.

In the end, the discovery of these five new particles could be a crucial step along the road towards a Theory of Everything (ToE), or just another piece in the very big puzzle that is our existence. Stay tuned to see which!

Further Reading: CERN, LHCb, arXiv

Eye Opening Numbers On Space Debris

Still image taken from a movie, Space debris ? a journey to Earth, to be released April 18th, 2017. Credit: ESA

Orbital debris, otherwise known as “space junk”, is a major concern. This massive cloud that orbits the Earth is the result of the many satellites, platforms and spent launchers that have been sent into space over the years. And as time went on, collisions between these objects (as well as disintegrations and erosion) has created even more in the way of debris.

Aside from threatening satellites and posing a danger to long-term orbital missions – like the International Space Station – this situation could pose serious problems for future space launches. And based on the latest numbers released by the Space Debris Office at the European Space Operations Center (ESOC), the problem has been getting getting worse. Continue reading “Eye Opening Numbers On Space Debris”

What is Uranus Named After?

Uranus as seen by NASA's Voyager 2. Credit: NASA/JPL

The period known as the Scientific Revolution (ca. 16th to the 18th century) was a time of major scientific upheaval. In addition to advances made in mathematics, chemistry, and the natural sciences, several major discoveries were made in the field of astronomy. Because of this, our understanding of the size and structure of the Solar System was forever revolutionized.

Consider the discovery of Uranus. While this planet had been viewed on many occasions by astronomers in the past, it was only with the birth of modern astronomy that its true nature came to be understood. And with William Herschel‘s discovery in the 18th century, the planet would come to be officially named and added to the list of known Solar Planets.

Past Observations:

The first recorded instance of Uranus being spotted in the night sky is believed to date back to the 2nd century BCE. At this time, Hipparchos – the Greek astronomer, mathematician and founder of trigonometry – apparently recorded the planet as a star in his star catalogue (completed in 129 BCE).

Large floor mosaic from a Roman villa in Sassoferrato, Italy (ca. 200–250 CE). Aion (Uranus), the god of eternity, stands above Tellus (Gaia) and her four children (the seasons). Credit: Wikipedia Commons/Bibi Saint-Poi

This catalog was later incorporated into Ptolemy’s Almagest, which became the definitive source for Islamic astronomers and for scholars in Medieval Europe for over one-thousand years. During the 17th and 18th centuries, multiple recorded sightings were made by astronomers who catalogued it as being a star.

This included English astronomer John Flamsteed, who in 1690 observed the star on six occasions and catalogued it as a star in the Taurus constellation (34 Tauri). During the mid-18th century, French astronomer Pierre Lemonnier made twelve recorded sightings, and also recorded it as being a star. It was not until March 13th, 1781, when William Herschel observed it from his garden house in Bath, that Uranus’ true nature began to be revealed.

Discovery:

Herschel’s first report on the object was recorded on April 26th, 1781. Initially, he described it as being a “Nebulous star or perhaps a comet”, but later settled on it being a comet since it appeared to have changed its position in the sky. When he presented his discovery to the Royal Society, he maintained this theory, but also likened it to a planet.

Replica of Herschel’s Seven-foot Reflecting Telescope, located at the Herschel Museum of Astronomy. Credit: herschelmuseum.org.uk

As was recorded in the Journal of the Royal Society and Royal Astronomical Society on the occasion of his presentation:

“The power I had on when I first saw the comet was 227. From experience I know that the diameters of the fixed stars are not proportionally magnified with higher powers, as planets are; therefore I now put the powers at 460 and 932, and found that the diameter of the comet increased in proportion to the power, as it ought to be, on the supposition of its not being a fixed star, while the diameters of the stars to which I compared it were not increased in the same ratio. Moreover, the comet being magnified much beyond what its light would admit of, appeared hazy and ill-defined with these great powers, while the stars preserved that lustre and distinctness which from many thousand observations I knew they would retain. The sequel has shown that my surmises were well-founded, this proving to be the Comet we have lately observed.”

While Herschel would continue to maintain that what he observed was a comet, his “discovery” stimulated debate in the astronomical community about what Uranus was. In time, astronomers like Johann Elert Bode would conclude that it was a planet, based on its nearly-circular orbit. By 1783, Herschel himself acknowledged that it was a planet to the Royal Society.

Name and Meaning:

As he lived in England, Herschel originally wanted to name Uranus after his patron, King George III. Specifically, he wanted to call it Georgium Sidus (Latin for “George’s Star”), or the Georgian Planet. Although this was a popular name in Britain, the international astronomy community didn’t think much of it, and wanted to follow the historical precedent of naming the planets after ancient Greek and Roman gods.

These two pictures of Uranus — one in true color (left) and the other in false color — were compiled from images returned Jan. 17, 1986, by the narrow-angle camera of Voyager 2. Credit: NASA/JPL

Consistent with this, Bode proposed the name Uranus in a 1782 treatise. The Latin form of Ouranos, Uranus was the grandfather of Zeus (Jupiter in the Roman pantheon), the father of Cronos (Saturn), and the king of the Titans in Greek mythology. As it was discovered beyond the orbits of Jupiter and Saturn, the name seemed highly appropriate. As he would later write in his 1784 book, “From the Newly Discovered Planet“:

“Already in the pre-read at the local Natural History Society on 12th March 1782 treatise, I have the father’s name from Saturn, namely Uranus, or as it is usually with the Latin suffix, proposed Uranus, and have since had the pleasure that various astronomers and mathematicians, cited in their writings or letters to me approving this designation. In my view, it is necessary to follow the mythology in this election, which had been borrowed from the ancient name of the other planets; because in the series of previously known, perceived by a strange person or event of modern times name of a planet would very noticeable. Diodorus of Cilicia tells the story of Atlas, an ancient people that inhabited one of the most fertile areas in Africa, and looked at the sea shores of his country as the homeland of the gods. Uranus was her first king, founder of their civilized life and inventor of many useful arts. At the same time he is also described as a diligent and skilful astronomers of antiquity … even more: Uranus was the father of Saturn and the Atlas, as the former is the father of Jupiter.”

There were some holdouts to this new name, largely in Britain, where the name Georgium Sidus remained popular. Nevertheless, Herschel’s proposal would become universally accepted by 1850. Uranus was the only planet in the Solar System named after a god from Greek mythology, rather than using the Roman counterpart’s name. 

Other Names:

While Uranus remains the widely-recognized name for the Solar System’s seventh planet (and third gas giant), other cultures have recognized it by various other names. For example in traditional Chinese astronomy, it is known as Tianwángxing, which means literally “Sky King Star”.

Uranus. Image credit: Hubble
Uranus, as imaged by the Hubble Space Telescope. Credit: NASA/Hubble

The same name is recognized in the Korean, Japanese and Vietnamese astronomical traditions. To the Aztecs (and other Nahuatl-speaking peoples), Uranus was known as “Ilhuicateocitlalli” – named after the word for “sky” (“ilhuicatl”) – and also as “Xiuhteuccitlalli”, the Aztec god of fire, day, and heat. Many other cultures recognized Uranus in their mythological traditions and assigned various names.

The discovery of Uranus was one of several that would follow from the 18th century onward. In time, Neptune, the Asteroid Belt, Ceres, Vesta, Pluto and the Kuiper Belt would be added to the mix, thus creating a model of the Solar System that would endure until the early 21st century – when new bodies were discovered beyond the orbit that Neptune that would lead to the nomenclature debate.

We have written many interesting articles on Uranus here at Universe Today. Here’s The Planet Uranus, Ten Interesting Facts About Uranus, Why is Uranus on its Side?, Tilt of Saturn, and Who Discovered Uranus?

For more information, here’s an article from the Hubble educational site about the discovery of Uranus, and here’s NASA’s Solar System Exploration page on Uranus.

We have recorded an episode of Astronomy Cast just about Uranus. You can access it here: Episode 62: Uranus.

Sources:

Last Look At Mimas For A Long Time

Mosaic view of Mimas, created using images taken by the Cassini probe (and illuminated to show the full surface). Credit: NASA/JPL-Caltech/Space Science Institute

Since the Cassini mission arrived in the Saturn system in 2004, it has provided some stunning images of the gas giant and its many moons. And in the course of capturing new views of Titan’s dense atmosphere, Iapetus’ curious “yin-yang” coloration, and the water plumes and “tiger stripes” of Enceladus, it snapped the most richly-detailed images of Mimas ever seen.

But like all good things, Cassini’s days of capturing close-up images of Mimas are coming to an end. As of January 30th, 2017, the probe made its final close approach to the moon, and took the last of it’s close-up pictures in the process. In the future, all observations (and pictures) of Mimas will take place at roughly twice this distance – and will therefore be less detailed.

To be fair, these close approaches were a pretty rare event during the Cassini mission. Over the course of the thirteen years that the probe has been in the Saturn system, only seven flybys have taken place, occurring at distances of less 50,000 km (31,000 mi). At its closest approach, Cassini passed within 41,230 km (25,620 mi) of Mimas.

Second mosaic view of Mimas, showing illumination on only the Sun-facing side. Credit: NASA/JPL-Caltech/Space Science Institute

During this time, the probe managed to take a series of images that allowed for the creation of a beautiful mosaic. This mosaic was made from ten combined narrow-angle camera images, and is one of the highest resolution views ever captured of the icy moon. It also comes in two versions. In one, the left side of Mimas is illuminated by the Sun and the picture is enhanced to show the full moon (seen at top).

In the second version (shown above), natural illumination shows only the Sun-facing side of the moon. They also created an animation that allows viewers to switch between mosaics, showing the contrast. And as you can see, these mosaics provide a very detailed look at Mimas heavily-cratered surface, a well as the large surface fractures that are believed to have been caused by the same impact that created the Herschel Crater.

This famous crater, from which Mimas gets it’s “Death Star” appearance, was photographed during Cassini’s first flyby – which occurred on February 13th, 2010. Named in honor of William Herschel (the discoverer of Uranus, its moons Oberon, and Titania, and Saturn’s moons Enceladus and Mimas), this crater measures 130 km (81 mi) across, almost a third of Mimas’ diameter.

This mosaic, created from images taken by NASA’s Cassini spacecraft during its closest flyby of Saturn’s moon Mimas, looks straight at the moon’s huge Herschel Crater Credit: NASA/JPL

Its is also quite deep, as craters go, with walls that are approximately 5 km (3.1 mi) high. Parts of its floor reach as deep as 10 km (6.2 mi), and it’s central peak rises 6 km (3.7 mi) above the crater floor. The impact that created this crater is believed to have nearly shattered Mimas, and also caused the fractures visible on the opposite side of the moon.

It’s a shame we won’t be getting any more close ups of the moon’s many interesting features. However, we can expect a plethora of intriguing images of Saturn’s rings, which it will be exploring in depth as part of the final phase of its mission. The mission is scheduled to end on September 15th, 2017, which will culminate with the crash of the probe in Saturn’s atmosphere.

Further Reading: NASA

Zero2Infinity Successfully Test Launches Its Bloostar Prototype

Zero 2 Infinity's Bloostar being deployed from a balloon 25 km (15.5 mi) above the coast of Spain. Credit: zero2infinity.space

Founded in 2009, the private aerospace company Zero2Infinity – which is headquartered in Barcelona, Spain – was created with the vision of delivering orbital payloads and providing space tourism on a budget. But unlike your conventional aerospace companies – i.e. SpaceX, Blue Origin, Orbital ATK, etc – their plan is to do it all using high-altitude stratospheric balloons.

On March 1st, the Zero2Infinity team passed a major milestone, deploying a prototype “rockoon” craft from the National Institute of Aerospace Technology‘s (INTA) facility in El Arenosillo, Spain. Known as Bloostar, this two-stage craft (which consists of a balloon and a rocket) is one of the latest technologies seeking to drastically reduce the costs of launching people and payloads into space.

As the name would suggest, the Bloostar craft consists of a first-stage balloon that carries a launch vehicle to altitudes of about 40 km (25 mi), where it is then engages its engine. By bringing a rocket to an attitude that is twice the cruising altitude of commercial aircraft, rockoons are capable of reducing the size of rockets and the amount of propellant needed to place payloads into orbit.

The launch vehicle itself is composed of a set of liquid fuel engines that are arranged in a concentric torus-configuration, which are then attached to the central payload. Each torus works as a stage during the rocket’s ascent, which are ignited once it reaches deployment altitude. After all the rocket stages are are finished deploying the payload, they all return to Earth with the balloon where they are recovered.

In this respect, the Bloostar employs technology that is similar to what United Launch Alliance is exploring with the proposed mid-air recovery of their Vulcan rockets’ engines. But the largest cost-cutting measure arises from the fact that the ignition phase does not start until the rocket is at an altitude that puts its beyond 95% of the mass of the Earth’s atmosphere.

This also allows for additional flexibility with launches since it means getting above inclement weather, and also ensures that polluting emissions are not added to the lower atmosphere. The use of several torus-shaped stages reduces the chance of damage occurring to the launch vehicle on re-entry, since several small stages experience less in the way of air friction and heat than larger rocket states.

There is the added benefit of there being less chance of damage. Oftentimes, satellites have fold-out solar panels and science instruments that have to be tucked away to be able to fit inside the cargo hold of a launch vehicle. But with the Bloostar, they can be attached to the flat front end, and will experience less in the way of launch stress since they are floated into space instead of accelerated to escape velocity.

 

Diagram showing the various stages in the launch of he Bloostar. Credit: zero2infinity.space

For the sake of their test flight, the Bloostar’s first-stage was elevated to an altitude of 25 km (15.5 mi) above sea level, a little over halfway towards their maximum deployment height. Once there, the launch vehicle conducted a successful ignition test. In addition to being a crucial milestone in the development of the prototype, the flight provided an opportunity to test several key subsystems and steps that will come into play.

These included the craft’s telemetry systems, which needed to be tested in space. There was also the controlled ignition sequence and stabilization systems of the rocket, the launch sequence, the deployment of its parachute deployment, and finally, recovery of the engines at sea. And according to a news release issued by the company on Monday, March 13th, “All these goals were achieved in full.”

This test was a first for the aerospace industry, as Zero2Infinity is currently the only company using stratospheric balloons as a first-stage vehicle. And already, the company states that it has garnered its fair share of interest from leading satellite developers, claiming that they have “gathered upwards of 250 million Euros in Letters of Intent for future launches.”

In addition to Bloostar, the company also has a space tourism program in the works. Known as “Bloon“, this service will offer clients the ability to travel to near-space aboard a stratospheric balloon for a chance to see Earth from suborbit. The purpose here is not just leisure, but to inspire people to appreciate the planet as a whole and help to protect it.

And then there’s Elevate, which is the company’s service for launching communications and weather-monitoring satellites, science experiments, stratospheric platforms, and other payloads to sub-orbital space. One of the more interesting packages they deployed in recent years was a Barbie doll in October of 2016, as part of Mattel’s “Barbie to Space” PR campaign.

There is no doubt that the commercial aerospace sector (aka. NewSpace) plays an important role in the era of renewed space exploration. Whereas the Space Race was characterized by fierce competition between two rival superpowers and their respective federal space agencies, the new era is characterized by cooperation between multiple space agencies and (for he most part) healthy competition in the private sector.

With the development of reusable rockets, reusable launch components, and now reusable “rockoons”, the costs of exploiting Low-Earth Orbit are dropping, and space itself is becoming far more accessible.

Further Reading: zero2infinity

Russia Recruiting For Its Moon Bound Cosmonauts

Statue of Yuri Gagarin, the first man in space, at the Baikonur Cosmodrome. Credit: AFP

 

Roscosmos has certainly come a long way in the past few decades. After facing an uncertain future in the 1990s, the federal space agency has rebounded to become a major player in space and a crucial partner in the International Space Station. And in the coming years, Roscosmos hopes to expand its reach further, with missions planned to the Moon and even Mars.

Towards this end, on Tuesday, March 14th, the agency announced that it is conducting a recruitment drive for new cosmonauts. All are welcome, the agency stressed, to apply to become the next-generation of space explorers (provided they meet the criteria). And if all goes as planned, a few lucky applicants will be the first members of the Russian space program to “fly to the Moon.”

Understandably, Roscosmos is hoping to jump start its space exploration program again and recapture the momentum it enjoyed during the Soviet Era. In addition to Sputnik and sending the first man and woman into space (as part of the Vostok program), the Soviet space program also produced a reusable spacecraft by the 1980s that was similar to the Space Shuttle (known as the Buran program).

Rollout and Erection of Vostok 1, the flight that took the first man (Yuri Gagarin) into space on April 12th, 1961. Credits: alldayru.com

Unfortunately, with budget cuts during this decade and the fall of the Soviet Union in 1991, several changes had to be made. For one, Roscosmos needed to turn to commercial satellite launches and space tourism in order to make up the difference in its funding. In addition, some observers have cited how Russia’s financial commitment to  the ISS has had a detrimental effect on other programs.

It is little wonder then why Russian wants to embark on some serious missions in the coming decades, ones which will reestablish it as a leader in space exploration. Intrinsic to this is a proposed crewed mission to the Moon, which is scheduled to take place in 2031. Roscosmos has also been developing the next-generation spacecraft that will replace the Soyuz-TMA, which has been the workhorse of the space program since the Soviet era.

Known as the the Federatsiya (Federation) capsule, this vehicle is scheduled to make its first crewed flight to space sometime in 2023 from the Vostochny cosmodrome in the Russian far east. As you can see from the images, it bears a striking resemblance to the Orion capsule. Unveiled at the 12th International Aviation and Space Salon in Moscow (MAKS-2015), this capsule will carry the first Russian cosmonauts to the Moon.

All they need now is fresh blood to make the journey. Hence why they are conducting their first recruitment drive in five years, which is the second drive to be is open to all people – not just military pilots, but also those working in the space industry. This time around, Roscosmos is looking for 6 to 8 new recruits who will train in how to fly the next-generation spaceships and make Russia’s long-awaited lunar landing.

The Federatsiya crew capsule being unveiled at the 12th International Aviation and Space Salon in Moscow. Credit: Wikipedia Commons/Roscosmos

As Sergei Kiralyov (Roscosmos’ Executive Director of Manned Programs) was quoted by RIA Novosti as saying, “There will be no discrimination based on skin colour or gender.” The criteria for these applicants include an age limit of 35, a height of between 1 m 50 cm – 1 m 90 cm (4’11” and 6’2″), and a weight of no more than 90 kilograms (~198 pounds).

The criteria also stress physical fitness, and claim that applicants must be able to cross-country ski for 5 km (~3 mi). They must also pass a series of psychological and physical tests (which include gynaecological examinations for women). In terms of skills, Roscosmos is seeking individuals who have an engineering degree, pilot training, experience in the aviation industry, and IT skills. Knowledge of a foreign language is also a plus (other than Russian, of course!).

“Recruitment of cosmonauts will take place starting from today, March 14, will take place before the end of the year. The results would be summed up in the end of December,” said Roscosmos’ First Deputy Director General Alexander Ivanov. Roscosmos also stressed that all those who are interested must apply by post or in person at the Star City astronaut training center outside Moscow (with three passport-sized photos included).

So if you speak Russian, are interesting in becoming part of the next-generation of cosmonauts, meet the requirements, or just want to go to the Moon, you might want to consider throwing your hat into the ring! Down the road, Roscosmos also has plans to conduct crewed missions to Mars between 2040 and 2060. These are expected to take place only after missions to the Moon are complete, which may include the creation of a lunar outpost.

Further Reading: Phys.org, AFP

How Far is Venus From the Sun?

On June 5th, 2012, the NASA/JAXA Hinode mission captured these stunning views of the transit of Venus. Credit: JAXA/NASA/Lockheed Martin

Earth and Venus are often called “sister planets” because they share some key characteristics. Like Earth, Venus is a terrestrial planet (i.e. composed of silicate minerals and metals) and orbits within our Sun’s habitable zone. But of course, they are also some major differences between them, like the fact that Venus’ is atmosphere is extremely dense and the hottest in the Solar System.

This is particularly interesting when you consider that Venus is not the closest planet to our Sun (that would be Mercury). In fact, its distance from the Sun is just over 70% the distance between Earth and the Sun. And due to its low eccentricity, there is very little variation in its distance during the course of its orbital period.

Perihelion and Aphelion:

While all planets follow an elliptical orbit, Venus’s orbit is the least eccentric of any of the Solar Planets. In fact, with an eccentricity of just 0.006772 , its orbit is the closest to being circular of any of the planets. It’s average distance (semi-major axis) from the Sun is 108,208,000 km (67,237,334 mi), and ranges from 107,477,000 km (66,783,112 mi) at perihelion to 108,939,000 km (67,691,556 mi) at aphelion.

Earth and Venus’ orbit compared. Credit: Sky and Telescope

To put it another way, Venus orbits the Sun at an average distance of 0.723 AU, which ranges from 0.718 AU at its closest to 0.728 AU at its farthest. Compare this to Earth’s eccentricity of 0.0167, which means that it orbits the Sun at an average distance of 1 AU, and that this distance ranges between 0.983 and 1.0167 AUs during its orbital period.

To express that in precise terms, the Earth orbits the Sun at an average distance of 149,598,023 km (92,955,902 mi), and varies between a distance of 147,095,000 km (91,401,000 mi) at perihelion to a distance of 152,100,000 km (94,500,000 mi) at aphelion.

Mars, by contrast, orbits the Sun at an average distance of 227,939,200 km (141,634,852 mi), or 1.52 AU. But due to its high eccentricity of 0.0934, it ranges from a distance of 206,700,000 km (128,437,425 mi) at perihelion to 249,200,000 km (154,845,700 mi) at aphelion – or between 1.38 to 1.666 AUs.

Mercury, meanwhile, has the highest eccentricity of any planet in the Solar System – a surprising 0.2056. While it’s average distance from the Sun is 57,909,050 km (35,983,015 mi), or 0.387 AU, it ranges from 46,001,200 km (28,583,820 mi) at perihelion to 69,816,900 km (43,382,210 mi) at aphelion – or 0.3075 to 0.4667 AUs.

Animated diagram showing the spacing of the Solar Systems planet’s, the unusually closely spaced orbits of six of the most distant KBOs, and the possible “Planet 9”. Credit: Caltech/nagualdesign

Hence, you might say Venus is something of an oddity compared to its fellow-terrestrial planets. Whereas they all orbit our Sun with a certain degree of eccentricity (from fair to extreme), Venus is the closest to orbiting in a circular pattern. And with an orbital velocity of 35.02 km/s (126,072 km/h; 78,337.5 mph), Venus takes 224.7 Earth days to complete a single orbit around the Sun.

Retrograde Motion:

Another oddity of Venus is the peculiar nature of its rotation. Whereas most objects in our Solar System have a rotation that is in the same direction as their orbit around the Sun, Venus’ rotation is retrograde to its orbit. In other words, if you could view the Solar System from above the Sun’s northern polar region, all of the planets would appear to be orbiting it in a counter-clockwise direction.

They would also appear to be rotating on their axis in the same counter-clockwise direction. But Venus would appear to be slowly rotating in a clockwise direction, taking about 243 days to complete a single rotation. This is not only the slowest rotation period of any planet, it also means that a sidereal day on Venus lasts longer than a Venusian year.

A popular theory states that this is due to two major impacts taking place between Venus and a series protoplanets in the distant past. Much like the impact that is believed to have created the Moon (between Earth and Theia), the first of these impact would have created a moon in orbit of Venus, while a second (10 million years later) would reverseed its rotation and caused the moon to de-orbit.

Artist’s concept of a collision between proto-Earth and Theia, believed to happened 4.5 billion years ago. Credit: NASA

Every planet in our Solar System has is shares of quirks, and Venus is no exception. She’s “Earth’s Sister”, and she’s prone to extreme temperatures that do not vary. And her orbit is the most stable of any planet, also with very little variation. You might say Venus is the extremely hot-tempered sibling of Earth, and very straight-laced to boot!

We have written many articles about the orbits of the planets here at Universe Today. Here’s How Far are the Planets from the Sun?, How Far is Mercury from the Sun?, How Far is the Earth from the Sun?, How Far is the Moon from the Sun?, How Far is the Asteroid Belt from the Sun?, How Far is Jupiter from the Sun?, How Far is Saturn from the Sun?, How Far is Uranus from the Sun?, How Far is Neptune from the Sun?, and How Far is Pluto from the Sun?

If you’d like more information on Venus, check out Hubblesite’s News Releases about Venus, and here’s a link to NASA’s Solar System Exploration Guide on Venus.

We’ve also recorded an entire episode of Astronomy Cast all about Venus. Listen here, Episode 50: Venus.

Sources:

NASA Brings Trappist-1 Into Focus… Kinda Sorta

TRAPPIST-1 is probably the most well-known ultra-cool, or red dwarf, star. It is host to several rocky, roughly Earth-sized planets. Astronomers think it's no accident that ultra-cool stars and red dwarfs are host to so many smaller, rocky planets, and they hope that SPECULOOS will find them. Credit: NASA/JPL-Caltech
TRAPPIST-1 is probably the most well-known ultra-cool, or red dwarf, star. It is host to several rocky, roughly Earth-sized planets. Astronomers think it's no accident that ultra-cool stars and red dwarfs are host to so many smaller, rocky planets, and they hope that SPECULOOS will find them. Credit: NASA/JPL-Caltech

On February 22nd, 2017, NASA announced the discovery of a seven-planet system around the red dwarf star known as TRAPPIST-1. Since that time, a number of interesting revelations have been made. For starters, the Search for Extra-Terrestrial Intelligence (SETI) recently announced that it was already monitoring this system for signs of advanced life (sadly, the results were not encouraging).

In their latest news release about this nearby star system, NASA announced the release of the first images taken of this system by the Kepler mission. As humanity’s premier planet-hunting mission, Kepler has been observing this system since December 2016, a few months after the existence of the first three of its exoplanets was announced.

Continue reading “NASA Brings Trappist-1 Into Focus… Kinda Sorta”

Trump’s NASA Authorization Act In All Its Glory

NASA's Journey to Mars. NASA is developing the capabilities needed to send humans to an asteroid by 2025 and Mars in the 2030s. Credit: NASA/JPL

It’s no secret that NASA has had its share of worries with the Trump administration. In addition to being forced to wait several months to get a sense of the administration’s priorities, the space agency has also had to contend with proposed cuts to its Earth Observation and climate monitoring programs. But one thing which does not appear to be threatened is NASA’s “Journey to Mars“.

In accordance with the National Aeronautics and Space Administration Transition Authorization Act of 2017, the Trump administration has finally committed to funding NASA’s plans for deep space human exploration in the coming decades, and to the tune of $19.5 billion. Central to these plans is the proposed crewed mission to Mars, which is scheduled to take place by 2033.

The Act was introduced to Congress back in February and presented to President Trump for approval on Tuesday, March. 9th. Consistent with the Space Administration Authorization Act of 2010 and the NASA Transition Authorization Act of 2016, this bill approved of $19.5 billion in funding for NASA for fiscal year 2017, much of which was earmarked for the continuation of NASA’s “Journey to Mars”.

NASA has unveiled a new exercise device that will be used by Orion crews to stay healthy on their mission to Mars. Credit: NASA

In addition to maintaining the US government’s commitment “to extend humanity’s reach into deep space, including cis-lunar space, the Moon, the surface and moons of Mars, and beyond”, the Act also expressed the need for a continued commitment to the International Space Station and the utilization of Low Earth Orbit, and other related space ventures.

However, it is Section. 431, Subtitle C – Journey to Mars, that contains all the articles that are of particular interest to space enthusiasts – as these deal with the planned missions to Mars. Article 432, titled “Human Exploration Roadmap”, specifically states that:

“The Administrator shall develop a human exploration roadmap, including a critical decision plan, to expand human presence beyond low-Earth orbit to the surface of Mars and beyond, considering potential interim destinations such as cis-lunar space and the moons of Mars.

This roadmap, according to the Act, will include all the science and exploration goals that were outlined in the 2014 report, “Pathways to Exploration: Rationales and Approaches for a U.S. Program of Human Space Exploration”, which was prepared by the National Academies of Sciences, Engineering, and Medicine’s Committee on Human Spaceflight.

Artist concept of NASA’s Space Launch System (SLS) 70-metric-ton configuration launching to space. Credit: NASA/MSFC

In addition, they cite the many plans prepared by NASA and other advocates for Mars exploration over the years. These include “The Global Exploration Roadmap” (2013), “NASA’s Journey to Mars – Pioneering Next Steps in Space Exploration” (2015), the JPL’s “Minimal Architecture for Human Journeys to Mars” (2015), and Explore Mars’ “The Humans to Mars Report 2016“.

The Space Launch System (SLS), the Orion Space Capsule, a deep space habitat, and other capabilities are cited as crucial technologies. Other technologies that are identified are “space suits, solar electric propulsion, deep space habitats, environmental control life support systems, Mars lander and ascent vehicle, entry, descent, landing, ascent, Mars surface systems, and in-situ resource utilization.”

And last, but not least, is the need to pursue robotic and crewed missions that are intended to test these technologies – aka. Exploration Mission-1 (EM-1) and Exploration Mission-2 (EM-2). The former mission (which is scheduled for launch on September 30th, 2018) will be the first launch of the SLS with the Orion Capsule on-board, and will involve an uncrewed Orion being sent on a translunar mission.

Exploration Mission-2 (which is expected to launch in August of 2021) will be consists of a crew of four astronauts conducting another flight around the Moon and returning to Earth. Other crewed explorations are expected to follow during the 2020s, which may or may not include the crewed exploration of an asteroid towed into lunar orbit (as part of the Asteroid Redirect Mission, or ARM).

Here too, the Act was consistent with the NASA Transition Authorization Act of 2016. Based on growing budget assessments and the judgement that the benefits of “the Asteroid Robotic Redirect Mission have not been demonstrated to Congress to be commensurate with the cost”, the Act recommends that NASA select a more “cost-effective” option for testing the Orion capsule.

Aside from testing the components and developing the expertise necessary for a crewed mission to Mars, these mission will also establish an all-important “launch cadence”. In other words, NASA hopes to begin conducting regular launches using the SLS between 2021 and 2023, which will be key to restarting crewed exploration of the Solar System.

Of course, the Act also emphasizes the need for continued research into the potential health risks, which are currently being performed aboard the ISS. These include the dangers of exposure to radiation, the long-term effects of time spent in microgravity environments (i.e. muscle degeneration, loss of bone density, organ degeneration, and loss of eyesight), and efforts to mitigate them.

Of course, critics of the Act cite the adjustments made to spending on Earth sciences and heliophysics. In addition, this funding is only for the coming year, and future commitments will need to be made to ensure that the “Journey to Mars” can happen in the time frame provided. But the Act passed with almost unanimous support, and seems to have confirmed what many observers claimed about the space priorities of a Trump administration.

Proponents of space exploration and a mission to Mars can therefore rest easy, as it seems that both are safe for another year. As for Earth science and research, which are intrinsic to helping us predict the effects of climate change, that’s another battle!

Further Reading: congress.gov