OrbitalHub

NASA dicit:

Scheduled to launch in the mid-2020s, the Nancy Grace Roman Space Telescope, formerly known as WFIRST, will function as Hubble’s wide-eyed cousin. While just as sensitive as Hubble’s cameras, the Roman Space Telescope’s 300-megapixel Wide Field Instrument will image a sky area 100 times larger. This means a single Roman Space Telescope image will hold the equivalent detail of 100 pictures from Hubble.

The mission’s wide field of view will allow it to generate a never-before-seen big picture of the universe, which will help astronomers explore some of the greatest mysteries of the cosmos, like why the expansion of the universe seems to be accelerating. Some scientists attribute the speed-up to dark energy, an unexplained pressure that makes up 68% of the total content of the cosmos.

The Wide Field Instrument will also allow the Roman Space Telescope to measure the matter in hundreds of millions of distant galaxies through a phenomenon dictated by Einstein’s relativity theory. Massive objects like galaxies curve space-time in a way that bends light passing near them, creating a distorted, magnified view of far-off galaxies behind them. The Roman Space Telescope will paint a broad picture of how matter is structured throughout the universe, allowing scientists to put the governing physics of its assembly to the ultimate test.

The Roman Space Telescope can use this same light-bending phenomenon to study planets beyond our solar system, known as exoplanets. In a process called microlensing, a foreground star in our galaxy acts as the lens. When its motion randomly aligns with a distant background star, the lens magnifies, brightens and distorts the background star. The Roman Space Telescope’s microlensing survey will monitor 100 million stars for hundreds of days and is expected to find about 2,500 planets, well targeted at rocky planets in and beyond the region where liquid water may exist.

These results will make the Roman Space Telescope an ideal companion to missions like NASA’s Kepler and the upcoming Transiting Exoplanet Survey Satellite (TESS), which are designed to study larger planets orbiting closer to their host stars. Together, discoveries from these three missions will help complete the census of planets beyond our solar system. The combined data will also overlap in a critical area known as the habitable zone, the orbiting distance from a host star that would permit a planet’s surface to harbor liquid water — and potentially life.

By pioneering an array of innovative technologies, the Roman Space Telescope will serve as a multipurpose mission, formulating a big picture of the universe and helping us answer some of the most profound questions in astrophysics, such as how the universe evolved into what we see today, its ultimate fate and whether we are alone.

Video credit: NASA’s Goddard Space Flight Center
Scott Wiessinger (USRA): Lead Producer
Claire Andreoli (NASA/GSFC): Lead Public Affairs Officer
Barb Mattson (University of Maryland College Park): Narrator
Francis Reddy (University of Maryland College Park): Science Writer
Michael Lentz (USRA): Animator
Chris Meaney (KBRwyle): Animator
Adriana Manrique Gutierrez (USRA): Animator
Scott Wiessinger (USRA): Animator
Scott Wiessinger (USRA): Editor

Wikipedia dicit:

The Solar and Heliospheric Observatory (SOHO) is a spacecraft built by a European industrial consortium led by Matra Marconi Space (now Airbus Defence and Space) that was launched on a Lockheed Martin Atlas II AS launch vehicle on December 2, 1995 to study the Sun. SOHO has also discovered over 3,000 comets. It began normal operations in May 1996. It is a joint project of international cooperation between the European Space Agency (ESA) and NASA. Originally planned as a two-year mission, SOHO continues to operate after over 25 years in space: the mission is extended until the end of 2020 with a likely extension until 2022.

In addition to its scientific mission, it is a main source of near-real-time solar data for space weather prediction. Along with Wind, ACE and DSCOVR, SOHO is one of four spacecraft in the vicinity of the Earth–Sun L1 point, a point of gravitational balance located approximately 0.99 astronomical unit (AU)s from the Sun and 0.01 AU from the Earth. In addition to its scientific contributions, SOHO is distinguished by being the first three-axis-stabilized spacecraft to use its reaction wheels as a kind of virtual gyroscope; the technique was adopted after an on-board emergency in 1998 that nearly resulted in the loss of the spacecraft.

Video credit: NASA Goddard

Blue Origin dicit:

The Blue Origin National Team, which includes Lockheed Martin, Northrop Grumman, and Draper, was selected by NASA to begin to develop the Artemis Human Landing System.

Using existing and in development technologies provides the head start needed to meet NASA’s goal of landing at the South Pole of the Moon. Lockheed Martin’s Ascent Element is based on Orion; Northrop Grumman’s Transfer Element is based on Cygnus; and Blue Origin’s Descent Element is based on the Blue Moon lander and BE-7 engine, which has been in development for several years.

Video credit: Blue Origin

Wikipedia dicit:

Ingenuity (also known as the Mars Helicopter) is a robotic helicopter that is planned to be used to test the technology to scout interesting targets on Mars, and help plan the best driving route for future Mars rovers. The small drone helicopter is planned for deployment in 2021 from the Perseverance rover as part of the Mars 2020 mission. It is expected to fly up to five times during its 30-day test campaign, early in the rover’s mission, as it is primarily a technology demonstration. Each flight is planned to take no more than three minutes, at altitudes ranging from 3 to 10 m above the ground. It could potentially cover a distance of up to 300 metres (980 ft) per flight. It can use autonomous control and communicate with the Perseverance rover directly after each landing. If it works as expected, NASA could build on the design for future Mars aerial missions.

Video credit: NASA/JPL-Caltech

Wikipedia dicit:

The Lunar Gateway is an in-development mini-space station in lunar orbit intended to serve as a solar-powered communication hub, science laboratory, short-term habitation module, and holding area for rovers and other robots. It is expected to play a major role in NASA’s Artemis program, after 2024.

While the project is led by NASA, the Gateway is meant to be developed, serviced, and utilized in collaboration with commercial and international partners. It will serve as the staging point for both robotic and crewed exploration of the lunar south pole, and is the proposed staging point for NASA’s Deep Space Transport concept for transport to Mars. The science disciplines to be studied on the Gateway are expected to include planetary science, astrophysics, Earth observations, heliophysics, fundamental space biology, and human health and performance.

Gateway development includes all of the International Space Station partners: ESA, NASA, Roscosmos, JAXA, and CSA. Construction is planned to take place in the 2020s. The International Space Exploration Coordination Group (ISECG), which is composed of more than 14 space agencies including all major ones, has concluded that Gateway will be critical in expanding a human presence to the Moon, Mars, and deeper into the Solar System.

Video credit: NASA’s Kennedy Space Center

NASA dicit:

Using the most advanced Earth-observing laser instrument NASA has ever flown in space, scientists have made precise, detailed measurements of how the elevation of the Greenland and Antarctic ice sheets have changed over 16 years.

The results provide insights into how the polar ice sheets are changing, demonstrating definitively that small gains of ice in East Antarctica are dwarfed by massive losses in West Antarctica. The scientists found the net loss of ice from Antarctica, along with Greenland’s shrinking ice sheet, has been responsible for 0.55 inches (14 millimeters) of sea level rise between 2003 and 2019 – slightly less than a third of the total amount of sea level rise observed in the world’s oceans.

Video credit: NASA’s Goddard Space Flight Center
Lead Producer: Ryan Fitzgibbons (USRA)
Lead Writer: Kate Ramsayer (Telophase)
Scientist: Thomas A. Neumann Ph.D. (NASA/GSFC)
Lead Scientists: Benjamin E. Smith (University of Washington Applied Physics Lab Polar Science Center)
Helen Amanda Fricker (Scripps Institution of Oceanography, University of California, San Diego)
Alex S. Gardner (NASA/JPL CalTech)
Lead Visualizer: Kel Elkins (USRA)
Lead Editor: Ryan Fitzgibbons (USRA)
Lead Narrator: LK Ward (USRA)
Lead Animator: Adriana Manrique Gutierrez (USRA)
Videographer: Jefferson Beck (USRA)