OrbitalHub

NASA dixit:

“NASA’s new laser instrument, the Global Ecosystem Dynamics Investigation, or GEDI, has advanced laser technology that will reveal the makeup of remote forest ecosystems around the globe. GEDI will soar above Earth at 17,150 miles per hour onboard the International Space Station. Its measurements of the height of leaves, branches, trees, and shrubs below its path will help scientists map the structure of forests and better understand how ecosystems are storing or releasing carbon.

GEDI’s lidar instrument sends laser pulses down to Earth, where they penetrate the globe’s temperate and tropical forests. The laser beams ricochet off the first thing they hit, which can be a leaf atop a dense canopy, a protruding branch, or the ground from which the forest emerges. The energy returned to the GEDI telescope on the International Space Station will provide an intricate three-dimensional map of forest canopies and carbon storage.

Led by the University of Maryland in collaboration with NASA’s Goddard Space Flight Center, GEDI has the highest resolution and densest sampling of any lidar every put in orbit. ”

Video Credit: NASA Goddard/Matthew Radcliff

Wikipedia dixit:

“The Ionospheric Connection Explorer (ICON) is a satellite designed to investigate changes in the Earth’s ionosphere. ICON will study the interaction between Earth’s weather systems and space weather driven by the Sun, and how this interaction drives turbulence in the upper atmosphere. It is hoped that a better understanding of this dynamic will mitigate its effects on communications, GPS signals, and technology in general. It is part of NASA’s Explorers program and will be operated by UC Berkeley’s Space Sciences Laboratory.

Once launched, ICON will perform a two-year mission to observe conditions in both the thermosphere and ionosphere. ICON will be equipped with four instruments: a Michelson interferometer, built by the United States Naval Research Laboratory, will measure the winds and temperatures in the thermosphere; an ion drift meter, built by UT Dallas, will measure the motion of charged particles in the ionosphere; and two ultraviolet imagers built at UC Berkeley will observe the airglow layers in the upper atmosphere in order to determine both ionospheric and thermospheric density and composition.

Many low-Earth orbiting satellites, including the International Space Station, fly through the ionosphere and can be affected by its changing electric and magnetic fields. The ionosphere also acts as a conduit for many communications signals, such as radio waves and the signals that make GPS systems work. The ionosphere is where space weather manifests, creating unpredicted conditions such as electric currents that can cause electrical charging of satellites, changing density that can affect satellite orbits, and shifting magnetic fields that can induce current in power systems, causing strain, disrupt communications and navigation or even blackouts. Improved understanding of this environment can help predict such events and improve satellite design.”

Video Credit: NASA

Wikipedia dixit:

“Rocket Lab is a private American aerospace manufacturer and smallsat launcher with a wholly owned New Zealand subsidiary. It has developed a suborbital sounding rocket named Ä€tea and currently operates a lightweight orbital rocket known as the Electron, which provides dedicated launches for smallsats and cubesats.

The Electron test program began in May 2017, with commercial flights announced by the company to occur at a price listed in early 2018 as US$5.7 million. Launching from Mahia Peninsula, New Zealand, the rocket’s test flights took place on 25 May 2017 and 21 January 2018, while its first commercial flight took place on 11 November 2018.

Rocket Lab was founded in 2006 by New Zealander Peter Beck, the company’s CEO and CTO. Internet entrepreneur and fellow New Zealander Mark Rocket was the seed investor and co-director from 2007 to 2011. In 2009, Rocket Lab claimed it had become the first private company in the Southern Hemisphere to reach space with the Ä€tea-1 sounding rocket. The payload was not recovered. This was not deemed necessary. As an instrumentation dart, the payload was not powered; its trajectory depended only on the boost phase of flight. The boost stage was recovered, and did have flight telemetry, on which the claim of reaching space was based.

In December 2010, Rocket Lab was awarded a U.S. government contract from the Operationally Responsive Space Office (ORS) to study a low cost space launcher to place CubeSats into orbit. This agreement with NASA enables the company to use NASA resources such as personnel, facilities, and equipment for commercial launch efforts.”

Video Credit: Rocket Lab

NASA dixit:

“This is an incredible aerial view of NASA’s Recovery Team and the US Navy practicing recovering a test version of the Orion crew capsule after it splashes down. Underway Recovery Test-7 is one in a series of tests to verify and validate procedures and hardware that will be used to recover the Orion spacecraft after it splashes down in the Pacific Ocean following deep space exploration missions.”

Video Credit: NASA

NASA dixit:

“A planetary science Ph.D. student at University College London’s Mullard Space Science Laboratory in the United Kingdom, has developed a new image-processing technique to mine through the wealth of data about comet tails. The findings offer the first observations of striations forming in the tails, and an unexpected revelation about the Sun’s effect on comet dust.

Understanding how dust behaves in the tail — how it fragments and clumps together — can teach scientists a great deal about similar processes that formed dust into asteroids, moons and even planets all those billions of years ago. With this study, scientists gain new insights to long-held mysteries. The work sheds light on the nature of striated comet tails from the past and provides a crucial lens for studying other comets in the future. But it also opens a new line of questioning: What role did the Sun have in our solar system’s formation and early history?”

Video Credit: NASA Goddard/Genna Duberstein

NASA dixit:

“Every year, the ozone hole over Antarctica reaches an annual maximum extent during southern winter. The depletion of ozone by chlorofluorocarbons (CFCs) happens faster at colder temperatures and slows down as temperatures warm, so each October, the ozone layer begins to heal again for the year.

Scientists from NASA and NOAA work together to track the ozone layer throughout the year and determine when the hole reaches its annual maximum extent. This year, the South Pole region of Antarctica was slightly colder than the previous few years, so the ozone hole grew larger. However, scientists from NASA have developed models to predict what the ozone layer would have looked like without the Montreal Protocol, which banned the release of CFCs. Although the 2018 hole was slightly larger than that of 2017 or 2016, it was still much smaller than it would have been without the Montreal Protocol.”

Video Credit: NASA