ESO: Moon-forming disk observed around exoplanet

A new report from the European Southern Observatory (ESO):

Astronomers make first clear detection of a moon-forming disc around an exoplanet

This image, taken with the Atacama Large Millimeter/submillimeter Array (ALMA), in which ESO is a partner, shows wide (left) and close-up (right) views of the moon-forming disc surrounding PDS 70c, a young Jupiter-like planet nearly 400 light-years away. The close-up view shows PDS 70c and its circumplanetary disc centre-front, with the larger circumstellar ring-like disc taking up most of the right-hand side of the image. The star PDS 70 is at the centre of the wide-view image on the left. Two planets have been found in the system, PDS 70c and PDS 70b, the latter not being visible in this image. They have carved a cavity in the circumstellar disc as they gobbled up material from the disc itself, growing in size. In this process, PDS 70c acquired its own circumplanetary disc, which contributes to the growth of the planet and where moons can form. This circumplanetary disc is as large as the Sun-Earth distance and has enough mass to form up to three satellites the size of the Moon.

Using the Atacama Large Millimetre/submillimeter Array (ALMA), in which the European Southern Observatory (ESO) is a partner, astronomers have unambiguously detected the presence of a disc around a planet outside our Solar System for the first time. The observations will shed new light on how moons and planets form in young stellar systems.

“Our work presents a clear detection of a disc in which satellites could be forming,”

says Myriam Benisty, a researcher at the University of Grenoble, France, and at the University of Chile, who led the new research published today in The Astrophysical Journal Letters.

“Our ALMA observations were obtained at such exquisite resolution that we could clearly identify that the disc is associated with the planet and we are able to constrain its size for the first time,”

she adds.

The disc in question, called a circumplanetary disc, surrounds the exoplanet PDS 70c, one of two giant, Jupiter-like planets orbiting a star nearly 400 light-years away. Astronomers had found hints of a “moon-forming” disc around this exoplanet before but, since they could not clearly tell the disc apart from its surrounding environment, they could not confirm its detection — until now.

In addition, with the help of ALMA, Benisty and her team found that the disc has about the same diameter as the distance from our Sun to the Earth and enough mass to form up to three satellites the size of the Moon.

But the results are not only key to finding out how moons arise.

“These new observations are also extremely important to prove theories of planet formation that could not be tested until now,”

says Jaehan Bae, a researcher from the Earth and Planets Laboratory of the Carnegie Institution for Science, USA, and author on the study.

Planets form in dusty discs around young stars, carving out cavities as they gobble up material from this circumstellar disc to grow. In this process, a planet can acquire its own circumplanetary disc, which contributes to the growth of the planet by regulating the amount of material falling onto it. At the same time, the gas and dust in the circumplanetary disc can come together into progressively larger bodies through multiple collisions, ultimately leading to the birth of moons.

This image, taken with the Atacama Large Millimeter/submillimeter Array (ALMA), in which ESO is a partner, shows a close-up view on the moon-forming disc surrounding PDS 70c, a young Jupiter-like gas giant nearly 400 light-years away. It shows this planet and its disc centre-front, with the larger circumstellar ring-like disc taking up most of the right-hand side of the image. The dusty circumplanetary disc is as large as the Sun-Earth distance and has enough mass to form up to three satellites the size of the Moon.

But astronomers do not yet fully understand the details of these processes.

“In short, it is still unclear when, where, and how planets and moons form,”

explains ESO Research Fellow Stefano Facchini, also involved in the research.

“More than 4000 exoplanets have been found until now, but all of them were detected in mature systems. PDS 70b and PDS 70c, which form a system reminiscent of the Jupiter-Saturn pair, are the only two exoplanets detected so far that are still in the process of being formed,”

explains Miriam Keppler, researcher at the Max Planck Institute for Astronomy in Germany and one of the co-authors of the study [1].

“This system therefore offers us a unique opportunity to observe and study the processes of planet and satellite formation,”

Facchini adds.

PDS 70b and PDS 70c, the two planets making up the system, were first discovered using ESO’s Very Large Telescope (VLT) in 2018 and 2019 respectively, and their unique nature means they have been observed with other telescopes and instruments many times since [2].

The latest high resolution ALMA observations have now allowed astronomers to gain further insights into the system. In addition to confirming the detection of the circumplanetary disc around PDS 70c and studying its size and mass, they found that PDS 70b does not show clear evidence of such a disc, indicating that it was starved of dust material from its birth environment by PDS 70c.

An even deeper understanding of the planetary system will be achieved with ESO’s Extremely Large Telescope (ELT), currently under construction on Cerro Armazones in the Chilean Atacama desert.

“The ELT will be key for this research since, with its much higher resolution, we will be able to map the system in great detail,”

says co-author Richard Teague, a researcher at the Center for Astrophysics | Harvard & Smithsonian, USA. In particular, by using the ELT’s Mid-infrared ELT Imager and Spectrograph (METIS), the team will be able to look at the gas motions surrounding PDS 70c to get a full 3D picture of the system.

Notes

[1] Despite the similarity with the Jupiter-Saturn pair, note that the disc around PDS 70c is about 500 times larger than Saturn’s rings.

[2] PDS 70b was discovered using the Spectro-Polarimetric High-contrast Exoplanet REsearch (SPHERE) instrument, while PDS 70c was found using the VLT’s Multi Unit Spectroscopic Explorer (MUSE). The two-planet system has been investigated using the X-shooter instrument too, also installed on ESO’s VLT.

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Videos: “Space to Ground” + Other ISS reports – July.16.2021

Here is the latest episode in NASA’s Space to Ground weekly report on activities related to the International Space Station:

** Space is Spicier: Peppers Growing on StationNASA’s Kennedy Space Center

On July 12, NASA astronaut Shane Kimbrough on the International Space Station added water to NASA’s Plant Habitat-04 (PH-04) experiment in the Advanced Plant Habitat (APH), the largest of NASA’s three plant growth chambers on the orbiting laboratory. This activated the experiment, which contains 48 Hatch chili pepper seeds recently sent to station. Astronauts on station and a team of researchers at Kennedy will work together to monitor the peppers’ growth for about four months before harvesting them. This will be one of the longest and most challenging plant experiments attempted aboard the orbital lab. The crew plans to eat some of the peppers and send the rest back to Earth for analysis. Some of the data collected from PH-04 will include the astronauts’ take on flavor and texture of the peppers, along with Scoville measurements to assess the spiciness of the peppers. A research team monitoring a control experiment on the ground at Kennedy will collect similar information for comparison. SpaceX’s 22nd commercial resupply services mission in June delivered PH-04 to the space station. Read the full feature and the fact sheet about the PH-04 experiment. Follow progress on social media. Feature: https://www.nasa.gov/feature/chile-pe… Fact Sheet: https://www.nasa.gov/content/plant-ha…

For information on the NuMex pepper Hatch Valley video footage, please contact New Mexico TRUE at www.newmexico.org

** Cool Flames Created Aboard International Space Station – July 14, 2021 – NASA Video

The hot flame created during a test for the Cool Flames Investigation with Gases experiment is shown burning. After the flame appears to extinguish, a cool flame is created. While too faint to be visible in real time during space station testing, the research team uncovered the presence of cool flames in the data.

** Expedition 65 Inflight with Harlem Link Education Group – July 9, 2021NASA Video

Aboard the International Space Station, ISS Expedition 65 Commander Aki Hoshide of the Japan Aerospace Exploration Agency (JAXA) and NASA Flight Engineer Shane Kimbrough answered pre-recorded questions from Harlem Link charter school students in New York July 8 in an educational in-flight events. The students represent all five boroughs of New York, ranging in age from pre-kindergarten to fifth grade. Hoshide and Kimbrough launched in April on the SpaceX Crew Dragon “Endeavour” for a planned six-month mission.

** Space Station Crew Answers Questions From New York State StudentsNASA Video

Expedition 65 – NASA Astronaut Megan McArthur and ESA Astronaut Thomas Pesquet answer questions from the Children’s Museum of Saratoga.

** ‘Intelligent’ robotic arm to launch with new space station moduleVideoFromSpace

European Robotic Arm (ERA) will be able to “move back and forward by itself, hand-over-hand between fixed base-points,” according to ESA, It will be launched to the International Space Station along with the ‘Nauka’ Russian Multipurpose Laboratory Module.

** WATCH Earth Images from the International Space Station.- July 12, 2021 space googlevesaire

** Spacewalk season timelapse, episode 3European Space Agency, ESA

Timelapse video made during ESA astronaut Thomas Pesquet’s second mission to the International Space Station, “Alpha”. ESA astronaut Thomas Pesquet and @NASA astronaut Shane Kimbrough performed three spacewalks in the span of 10 days to install two new solar arrays that will generate more electricity on the International Space Station. The third and final spacewalk for the duo happened on June 25 to finish installing the second pair of new solar arrays. This spacewalk proceeded without problems, and the two new solar arrays are already working and supplying power to the Space Station. The design of the new solar arrays will be used to power the lunar Gateway that will be built in an orbit around the Moon – the next outpost in space for the agencies that run the International Space Station.

** Science so cool it is freezing! European Space Agency, ESA

Interviews with the “Cold Stowage” team at @NASA‘s Kennedy Space Center in Florida, USA, that ensure science on the International Space Station stays cool. Many experiments run on the Space Station require freezing samples for analysis later on Earth, or are sent into space frozen and thawed out in orbit. The European-built MELFI (Minus Eighty Lab Freezer for ISS) keeps these samples at the right temperature. From a virus to algae or muscle biopsies, many samples have been sent and stored in space over a decade years that the freezers have been operating. The technology behind keeping the science cool in space has found its way back to Earth too, limiting losses when transporting liquid gas in tankers. Built by ESA and transferred to NASA and @JAXA | 宇宙航空研究開発機構, MELFI is a versatile storage freezer. The four compartments can be set at different temperatures ranging from −98 °C to +4 °C to preserve biological samples such as blood and urine that will be returned to Earth.

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ESO: Galactic star formation seen vividly in VLT/ALMA images

A new report from the European Southern Observatory (ESO):

Galactic fireworks:
new ESO images reveal stunning features of nearby galaxies

This image combines observations of the nearby galaxies NGC 1300, NGC 1087, NGC 3627 (top, from left to right), NGC 4254 and NGC 4303 (bottom, from left to right) taken with the Multi-Unit Spectroscopic Explorer (MUSE) on ESO’s Very Large Telescope (VLT). Each individual image is a combination of observations conducted at different wavelengths of light to map stellar populations and warm gas. The golden glows mainly correspond to clouds of ionised hydrogen, oxygen and sulphur gas, marking the presence of newly born stars, while the bluish regions in the background reveal the distribution of slightly older stars.   The images were taken as part of the Physics at High Angular resolution in Nearby GalaxieS (PHANGS) project, which is making high-resolution observations of nearby galaxies with telescopes operating across the electromagnetic spectrum.

A team of astronomers has released new observations of nearby galaxies that resemble colourful cosmic fireworks. The images, obtained with the European Southern Observatory’s Very Large Telescope (ESO’s VLT), show different components of the galaxies in distinct colours, allowing astronomers to pinpoint the locations of young stars and the gas they warm up around them. By combining these new observations with data from the Atacama Large Millimeter/submillimeter Array (ALMA), in which ESO is a partner, the team is helping shed new light on what triggers gas to form stars.

This image of the nearby galaxy NGC 1300 was obtained by combining observations taken with the Multi-Unit Spectroscopic Explorer (MUSE) on ESO’s Very Large Telescope (VLT) and with the Atacama Large Millimeter/submillimeter Array (ALMA), in which ESO is a partner. NGC 1300 is a spiral galaxy, with a bar of stars and gas at its centre, located approximately 61 million light-years from Earth in the constellation Eridanus. The image is a combination of observations conducted at different wavelengths of light to map stellar populations and gas. ALMA’s observations are represented in brownish-orange tones and highlight the clouds of cold molecular gas that provide the raw material from which stars form. The MUSE data show up mainly in gold and blue. The bright golden glows map warm clouds of mainly ionised hydrogen, oxygen and sulphur gas, marking the presence of newly born stars, while the bluish regions reveal the distribution of slightly older stars.  The image was taken as part of the Physics at High Angular resolution in Nearby GalaxieS (PHANGS) project, which is making high resolution observations of nearby galaxies with telescopes operating across the electromagnetic spectrum.

Astronomers know that stars are born in clouds of gas, but what sets off star formation, and how galaxies as a whole play into it, remains a mystery. To understand this process, a team of researchers has observed various nearby galaxies with powerful telescopes on the ground and in space, scanning the different galactic regions involved in stellar births.

“For the first time we are resolving individual units of star formation over a wide range of locations and environments in a sample that well represents the different types of galaxies,”

says Eric Emsellem, an astronomer at ESO in Germany and lead of the VLT-based observations conducted as part of the Physics at High Angular resolution in Nearby GalaxieS (PHANGS) project.

“We can directly observe the gas that gives birth to stars, we see the young stars themselves, and we witness their evolution through various phases.” 

Emsellem, who is also affiliated with the University of Lyon, France, and his team have now released their latest set of galactic scans, taken with the Multi-Unit Spectroscopic Explorer (MUSE) instrument on ESO’s VLT in the Atacama Desert in Chile. They used MUSE to trace newborn stars and the warm gas around them, which is illuminated and heated up by the stars and acts as a smoking gun of ongoing star formation.

The new MUSE images are now being combined with observations of the same galaxies taken with ALMA and released earlier this year. ALMA, which is also located in Chile, is especially well suited to mapping cold gas clouds — the parts of galaxies that provide the raw material out of which stars form.

By combining MUSE and ALMA images astronomers can examine the galactic regions where star formation is happening, compared to where it is expected to happen, so as to better understand what triggers, boosts or holds back the birth of new stars. The resulting images are stunning, offering a spectacularly colourful insight into stellar nurseries in our neighbouring galaxies.

“There are many mysteries we want to unravel,”

says Kathryn Kreckel from the University of Heidelberg in Germany and PHANGS team member.

“Are stars more often born in specific regions of their host galaxies — and, if so, why? And after stars are born how does their evolution influence the formation of new generations of stars?”

Astronomers will now be able to answer these questions thanks to the wealth of MUSE and ALMA data the PHANGS team have obtained. MUSE collects spectra — the “bar codes” astronomers scan to unveil the properties and nature of cosmic objects — at every single location within its field of view, thus providing much richer information than traditional instruments. For the PHANGS project, MUSE observed 30 000 nebulae of warm gas and collected about 15 million spectra of different galactic regions. The ALMA observations, on the other hand, allowed astronomers to map around 100 000 cold-gas regions across 90 nearby galaxies, producing an unprecedentedly sharp atlas of stellar nurseries in the close Universe.

This image of the nearby galaxy NGC 4303 was obtained by combining observations taken with the Multi-Unit Spectroscopic Explorer (MUSE) on ESO’s Very Large Telescope (VLT) and with the Atacama Large Millimeter/submillimeter Array (ALMA), in which ESO is a partner. NGC 4303 is a spiral galaxy, with a bar of stars and gas at its centre, located approximately 55 million light-years from Earth in the constellation Virgo. The image is a combination of observations conducted at different wavelengths of light to map stellar populations and gas. ALMA’s observations are represented in brownish-orange tones and highlight the clouds of cold molecular gas that provide the raw material from which stars form. The MUSE data show up mainly in gold and blue. The bright golden glows map warm clouds of mainly ionised hydrogen, oxygen and sulphur gas, marking the presence of newly born stars, while the bluish regions reveal the distribution of slightly older stars.    The image was taken as part of the Physics at High Angular resolution in Nearby GalaxieS (PHANGS) project, which is making high-resolution observations of nearby galaxies with telescopes operating across the electromagnetic spectrum.

In addition to ALMA and MUSE, the PHANGS project also features observations from the NASA/ESA Hubble Space Telescope. The various observatories were selected to allow the team to scan our galactic neighbours at different wavelengths (visible, near-infrared and radio), with each wavelength range unveiling distinct parts of the observed galaxies.

“Their combination allows us to probe the various stages of stellar birth — from the formation of the stellar nurseries to the onset of star formation itself and the final destruction of the nurseries by the newly born stars — in more detail than is possible with individual observations,”

says PHANGS team member Francesco Belfiore from INAF-Arcetri in Florence, Italy.

“PHANGS is the first time we have been able to assemble such a complete view, taking images sharp enough to see the individual clouds, stars, and nebulae that signify forming stars.”

The work carried out by the PHANGS project will be further honed by upcoming telescopes and instruments, such as NASA’s James Webb Space Telescope. The data obtained in this way will lay further groundwork for observations with ESO’s future Extremely Large Telescope (ELT), which will start operating later this decade and will enable an even more detailed look at the structures of stellar nurseries.

“As amazing as PHANGS is, the resolution of the maps that we produce is just sufficient to identify and separate individual star-forming clouds, but not good enough to see what’s happening inside them in detail,”

pointed out Eva Schinnerer, a research group leader at the Max Planck Institute for Astronomy in Germany and principal investigator of the PHANGS project, under which the new observations were conducted.

“New observational efforts by our team and others are pushing the boundary in this direction, so we have decades of exciting discoveries ahead of us.”

[ See also these interactive comparisons of galaxy images with and without the ALMA radio array data:

]

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Space non-profits receive $1M grants from Blue Origin’s Club for the Future foundation

Good news for space education and the promotion of space development and settlement. Nineteen space-related non-profits, including several space activist organizations, will each get $1M from  Blue Origin.

Blue Origin’s foundation, Club for the Future,
selects 19 space-based charities to each receive a $1 million grant

Today, Blue Origin’s foundation, Club for the Future, announced 19 non-profit charitable organizations will each be offered a $1 million grant to inspire future generations to pursue careers in STEM and help invent the future of life in space. The funds are made possible by the recent auction for the first paid seat on Blue Origin’s New Shepard rocket.

Each of the organizations selected have demonstrated a commitment to promote the future of living and working in space to inspire the next generation to explore space careers. They enhance Club for the Future’s ability to reach students, teachers, and communities, and to engage them in the excitement and adventure of innovation and space exploration.

“Our recent auction for the first seat on New Shepard resulted in a donation of $28 million to our non-profit foundation, Club for the Future,” said Bob Smith, Blue Origin CEO. “This donation is enabling Club for the Future to rapidly expand its reach by partnering with 19 organizations to develop and inspire the next generation of space professionals.  Our generation will build the road to space and these efforts will ensure the next generation is ready to go even further.”

The 19 organizations include:

  • AstraFemina is a collective of prominent leaders, including astronauts, academic professionals, and industry innovators, who have made a significant difference in the world by choosing diverse careers in STEM fields. Its mission is simple but powerful – to serve as role models to reinforce the message to today’s girls and young women that anything is possible and help bridge the gap between believing and achieving.
  • The AIAA Foundation, which is connected to the American Institute of Aeronautics and Astronautics (AIAA), inspires and supports the next generation of aerospace professionals. From classroom to career, the AIAA Foundation enables innovative K-12 and university programming, including STEM classroom grants, scholarships, conferences, and hands-on competitions.
  • The Astronaut Scholarship Foundation (ASF) provides merit-based scholarships for college students majoring in STEM programs at more than 44 partner universities. Founded by the Mercury astronauts, ASF selects more than 50 Astronaut Scholars each year. They also provide programs focused on career development skills and virtual family activities to inspire K-12 students to positively change and innovate our future.
  • The Brooke Owens Fellowship offers paid internships and mentorship for exceptional undergrad women and gender minorities in aerospace. Its spin-off, the Patti Grace Smith Fellowship, provides extraordinary Black students with their first work experience in the aerospace industry, personalized mentorship and a cohort of similarly driven and talented young Black people pursuing aerospace careers.
  • Challenger Center, created by the families of Space Shuttle Challenger STS-51L crew, serves more than 250,000 K-12 students each year with experiential, hands-on education programs. The 40 Challenger Learning Centers deliver in-classroom and virtual simulation-based programs to bring STEM subjects to life. Students role-play real world STEM careers and cultivate teamwork, problem-solving, and communication skills.
  • Higher Orbits delivers an experiential learning lab for secondary school students across the United States. It focuses on the multi-faceted worlds of space exploration, research and spaceflight in order to launch the next generation our world desires. The organization facilitates activities from the novice to advanced level, drawing from the Science Futures by Design curriculum at Higher Orbits, to promote STEAM and prepare students for academic and career success.
  • International Astronautical Federation (IAF) is the leading space advocacy body, including all leading space agencies, numerous companies, research institutions, universities, societies, associations, institutes and museums worldwide. It’s Emerging Space Leaders Grant Program (ESL), enables students and young professionals to participate in the International Astronautical Congress, the United Nations/IAF Workshop and Space Generations Congress.
  • The National Space Society (NSS) is dedicated to the creation of a spacefaring civilization that provides a citizen’s voice on space exploration, development, and settlement. Its mission is to promote social, economic, technological, and political change in order to expand civilization beyond Earth, to settle space and to use the resulting resources to build a hopeful and prosperous future for humanity.
  • SciArt Exchange uses a science-integrated-with-art approach to help change the world through science and technology education, collaboration and innovation. It supports, prepares and convenes people of all ages, backgrounds and affiliations to discuss, and potentially solve, space, science, and technology challenges by offering multi-disciplinary art contests, events, training, consulting, and community services.
  • Space Camp, located at the U.S. Space & Rocket Center, provides a one-of-a-kind experience for campers of all ages from every state and more than 70 countries. Its curriculum teaches STEM principles, emphasizing leadership, teamwork, fun and creativity. Program instruction is aligned to national science and math standards and framed with an immersive experience amidst a backdrop of humankind’s greatest technological achievements in space hardware.
  • Space Center Houston is dedicated to inspiring all generations through the wonders of space exploration. It is a leading science and space exploration learning center, the Official Visitor Center of NASA Johnson Space Center, a Smithsonian Affiliate and Certified Autism Center. Space Center Houston empowers teachers and students with access to immersive learning experiences where they solve real-world challenges of human space exploration.
  • The Space For Art Foundation works with children in hospitals and refugee centers around the world on its mission to unite a planetary community of children through the wonder of space exploration and the healing power of art. Through large-scale space-themed art projects, the Foundation aims to highlight the connection between personal and planetary health and raise awareness of our role as crewmates here on Spaceship Earth.
  • Space For Humanity is building a foundation for an inclusive future in space by organizing the planet’s first Sponsored Citizen Astronaut Program, where leaders from any walk of life can apply for an opportunity to go to space. Through its citizen spaceflight program, leadership training, and collaborative efforts to educate the public, Space for Humanity is setting the stage to create a better world, both here on Earth and throughout the cosmos.
  • Space Generation Advisory Council (SGAC), in support of the United Nations Program on Space Applications, is a global non-governmental organization and network which aims to focus on pragmatic space policy advice to policy makers based on the interests of students and young professionals interested in space from around the world. The SGAC network of members, volunteers and alumni has 16,000 members from more than 165 countries.
  • Students for the Exploration and Development of Space (SEDS) is an international student-led  organization whose purpose is to promote space exploration and development through educational and engineering projects. SEDS is fostering the development of future leaders and contributors in the expanding space industry through individual chapters, enabling students to be connected and create networks with each other.
  • Teachers in Space is an organization which stimulates student interest in STEM by providing teachers with extraordinary space science experiences and industry connections. As a facilitator of personal and hands-on professional development workshops for STEM teachers, it sparks a transfer of passion that prepares and encourages students to pursue further education and careers in the emerging space industry.
  • The Mars Society is an international organization devoted to furthering the exploration and settlement of Mars by both public and private means. Its activities include broad public outreach to spread its vision, STEM programs, student engineering design and Mars rover competitions, conferences, publications, and scientific projects including Mars Analog Research Stations to learn how we might best live, work, and explore on the Red Planet.
  • The Planetary Society has inspired millions of people to explore other worlds and seek other life. Led by CEO Bill Nye and powered by space enthusiasts around the globe, the Society works to advance space science and exploration through education, innovation, advocacy, and global collaboration. Its mission is to empower the world’s citizens to advance space science and exploration.
  • The Space Frontier Foundation is an organization comprised of a diverse, multinational array of space activists, scientists, engineers, media, political professionals, entrepreneurs, and passionate citizens focused on unleashing the power of free enterprise and leading a united humanity permanently into the Solar System. Through conferences, speakers, policy papers, awards and prizes, they are actively advancing the cause of “New Space.”

Club for the Future will use the remaining funds from the auction to continue its work on its space-focused curriculum and Postcards to Space program. For more information about Club for the Future, visit ClubforFuture.org.

Blue Origin’s First Human Flight will take place on July 20. For more details about the mission and how to watch the launch live, follow @BlueOrigin on Twitter or sign up for updates at BlueOrigin.com.

-Gradatim Ferociter

Space policy roundup – July.12.2021

A sampling of links to recent space policy, politics, and government (US and international) related space news and resource items that I found of interest (find previous space policy roundups here):

International space

Webcasts:

** China Performs Spacewalk at the Chinese Space Station, Plethora of Launches in a Single Week – Ep 41Dongfang Hour – YouTube

Hello and welcome to another episode of the Dongfang Hour China Space News Roundup! A kind reminder that we cover a lot more stories every week in our Newsletter (newsletter.dongfanghour.com).

This week, we discuss:
1) China’s 1st EVA with Tianhe (and 2nd ever Chinese EVA)
2) A Plethora of launches in a Single Week
3) Guangzhou & Tianjin Add Satellite Internet to their Development Plans

A summary of the program is provided here: Dongfang Hour China Aerospace News Roundup 5 July – 11 July 2021 – SpaceWatch.Global.

** Episode 42 – What is Going on With This Idea of Space PollutionSpace Thoughts (YouTube) – Space Law & Policy Solutions/Michael Listner

** T+193: Marcia Smith, SpacePolicyOnline.com – Main Engine Cut Off

Marcia Smith of SpacePolicyOnline.com joins me for a round up of space policy news, including how the Biden and Nelson administrations are doing so far, things that are being overlooked or sidelined, the Senate’s NASA Authorization bill, NASA’s Human Landing System contract and the battle for funding, the space tourism learning period, and we finish with a quick look at what China and Russia have been up to lately.

** The Space Cafe Podcast #31: Ian Carnelli, Preparing for the worst – SpaceWatch.Global

Episode 031 features a special guest Ian Carnelli. Next year, a small spacecraft will head for the double asteroid Didymos to slam into it with its brakes off. The name of the mission gives free rein to the imagination: Planetary Defense Mission. It is a joint mission between ESA and NASA, and it wants to test for the first time what has long been a topic in science fiction: can a deadly chunk of rock be deflected from its collision course with the earth or is a second event that took away the dinosaurs only a matter of time? The Planetary Defense Mission will find an answer. Whether it is the one we would like remains to be seen. Mission Director Ian Carnelli paints a fascinating picture of this unique mission.

** Space Policy and History Forum: The History and Politics of Space JunkNASA Video

The exponential rise in debris cluttering Earth orbits poses formidable technical, political, financial, and legal challenges, from threatening satellites and space stations to impacting Earth to potentially provoking international conflict. How is the space debris situation evolving? Who is responsible for the management of Earth orbit? How should we approach debris removal and growth mitigation? Can the history of orbital debris help us achieve a safe and sustainable future in space? Join the Smithsonian’s National Air and Space Museum and NASA for a virtual Space Policy and History Forum featuring a panel discussion on the politics of orbital debris within a historical context. Panelists include: • Jonathan McDowell, Astrophysicist, Harvard-Smithsonian Center for Astrophysics • Lisa Ruth Rand, Assistant Professor of History, California Institute of Technology • Gabriel Swiney, Attorney Advisor, International Space Lawyer, U.S. State Department Moderated by Bhavya Lal, Senior Advisor for Budget and Finance, NASA.

** The Space Show – Friday, July.9.2021Dr. Matthew Weinzierl, a Harvard space economist, discussed “commercial space through the eyes of an economist”. See the paper, The Commercial Space Age Is Here – Harvard Business Review by Matt Weinzierl and Mehak Sarang.

** Hotel Mars: – The John Batchelor Show/The Space Show – Wed. July.7.2021Leonard David talked with John Batchelor and Dr. David Livingston about the upcoming Virgin Galactic and Blue Origin suborbital spaceflights and about space tourism in general

** The Space Show – Tuesday, July.6.2021Aaron Bateman spoke about “national space security issues and history“.

** Registering Lunar Activities – Moon Dialogs Salon #14 – Moon Dialogs

This salon was part of our Sustainable Moon series and features the first public workshop of The Registration Project and featured a number of space law experts. The Registration Project was launched to address the shortcomings of existing law and practice regarding registration as humankind returns to the Moon. The Project is a joint venture of the Moon Village Association (MVA) and the Global Space Law Center (GSLC) at Cleveland State University.

** Insight – 3rd Summit for Space Sustainability | Secure World

** Space Café WebTalk – Katherine Courtney – 18. May 2021spacewatch. global – News Room – YouTube

During this week’s Space Café, SpaceWatch.Global publisher Torsten Kriening met with space strategist and former Chief Executive for the UK Space Agency, Katherine Courtney, to discuss space sustainability and her role as founder of education charity PrimarySpace.

Katherine is the current strategic adviser for Arqit, an encryption platform based in London. She was previously the regulator for UK License Space Operations and has worked with organisations such as Avascent, the Global Network on Sustainability in Space and MULTIPLY Space to create clear strategies, manage risks and multiply returns on innovation investment; bring government, researchers and businesses together to apply innovation to key policy aims; and support start-ups to scale-up.

This week, she and Torsten discuss the biggest risk of all – what will our contemporary use of space mean for future generations, and are we sleepwalking into the next catastrophe?

** Operating in a new space age: Does space security matter to industry?  Space Court Foundation – YouTube

** July 7, 2021 Zimmerman/Batchelor podcast – Behind The Black – Robert Zimmerman

** July 9, 2021 Zimmerman/Batchelor podcast – Behind The Black – Robert Zimmerman

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