OrbitalHub

Wikipedia dicit:

The Imaging X-ray Polarimetry Explorer, commonly known as IXPE, is a space observatory with three identical telescopes designed to measure the polarization of cosmic X-rays. The mission will study exotic astronomical objects and permit mapping the magnetic fields of black holes, neutron stars, pulsars, supernova remnants, magnetars, quasars, and active galactic nuclei. The high-energy X-ray radiation from these objects’ surrounding environment can be polarized – vibrating in a particular direction. Studying the polarization of X-rays reveals the physics of these objects and can provide insights into the high-temperature environments where they are created.

The IXPE mission was announced on 3 January 2017. It is being developed by NASA’s Small Explorer program (SMEX) and is slated for launch on 9 December 2021. The estimated cost of the mission and its two-year operation is US$188 million (the launch cost is US$50.3 million). The goal of the IXPE mission is to expand understanding of high-energy astrophysical processes and sources, in support of NASA’s first science objective in astrophysics: “Discover how the universe works”. By obtaining X-ray polarimetry and polarimetric imaging of cosmic sources, IXPE addresses two specific science objectives: to determine the radiation processes and detailed properties of specific cosmic X-ray sources or categories of sources; and to explore general relativistic and quantum effects in extreme environments.

During IXPE’s two-year mission, it will study targets such as active galactic nuclei, quasars, pulsars, pulsar wind nebulae, magnetars, accreting X-ray binaries, supernova remnants, and the Galactic Center.

Video credit: NASA

Wikipedia dicit:

Double Asteroid Redirection Test (DART) is a NASA space mission aimed at testing a method of planetary defense against near-Earth objects (NEO). It will deliberately crash a space probe into the double asteroid Didymos to test whether the kinetic energy of a spacecraft impact could successfully deflect an asteroid on a collision course with Earth. DART is a joint project between NASA and the Johns Hopkins Applied Physics Laboratory (APL), administered by NASA’s Planetary Defense Coordination Office, with several NASA laboratories and offices providing technical support. International partners, such as the space agencies of Europe, Italy, and Japan, are contributing to related or subsequent projects. DART was launched on 24 November 2021, at 06:21:02 UTC, with collision slated for 26 September 2022.

DART is an impactor, mass of 610 kg (1,340 lb), that hosts no scientific payload other than a Sun sensor, a star tracker, and a 20 cm (7.9 in) aperture camera (Didymos Reconnaissance and Asteroid Camera for Optical navigation – DRACO) based on Long-Range Reconnaissance Imager (LORRI) onboard New Horizons spacecraft to support autonomous navigation to impact the small asteroid’s moon at its center.

It is estimated that the impact of the 500 kg (1,100 lb) DART at 6.6 km/s (4.1 mi/s) will produce a velocity change on the order of 0.4 mm/s, which leads to a small change in trajectory of the asteroid system, but over time, it leads to a large shift of path. Over a span of millions of kilometers, the cumulative trajectory change would eliminate the risk of a previously-Earth-bound asteroid hitting Earth. The actual velocity change and orbital shift will be measured a few years later by a spacecraft called Hera that would do a detailed reconnaissance and assessment. Hera was approved in November 2019.

DART spacecraft uses the NEXT ion thruster, a type of solar electric propulsion. It will be powered by 22 m2 (240 sq ft) solar arrays to generate the ~3.5-kW needed to power the NASA Evolutionary Xenon Thruster–Commercial (NEXT-C) engine. The spacecraft’s solar arrays use a Roll Out Solar Array (ROSA) design, and this was tested on the International Space Station in June 2017 as part of Expedition 52, delivered to the station by the SpaceX CRS-11 commercial cargo mission.

Using ROSA as the structure, a small portion of the DART solar array is configured to demonstrate Transformational Solar Array technology, which has very-high-efficiency solar cells and reflective concentrators providing three times more power than current solar array technology.

The DART spacecraft is the first spacecraft to use a new type of high gain communication antenna, that is, a Spiral Radial Line Slot Array (RLSA). The antenna operates at the X-band NASA Deep Space Network (NASA DSN) frequencies of 7.2 and 8.4-GHz. The fabricated antenna exceeds the given requirements, agrees well simulations, and has been tested through environments resulting in a TRL-6 design.

Video credit: NASA/SpaceX

Wikipedia dicit:

The SpaceX South Texas launch site, referred to by SpaceX as Starbase, and also known as the Boca Chica launch site, is a private rocket production facility, test site, and spaceport constructed by SpaceX, located at Boca Chica approximately 32 km (20 mi) east of Brownsville, Texas, on the US Gulf Coast. When conceptualized, its stated purpose was “to provide SpaceX an exclusive launch site that would allow the company to accommodate its launch manifest and meet tight launch windows.” The launch site was originally intended to support launches of the Falcon 9 and Falcon Heavy launch vehicles as well as “a variety of reusable suborbital launch vehicles”, but in early 2018, SpaceX announced a change of plans, stating that the launch site would be used exclusively for SpaceX’s next-generation launch vehicle, Starship. Between 2018 and 2020, the site added significant rocket production and test capacity. SpaceX CEO Elon Musk indicated in 2014 that he expected “commercial astronauts, private astronauts, to be departing from South Texas,” and he foresaw launching spacecraft to Mars from the site.

Between 2012 and 2014, SpaceX considered seven potential locations around the United States for the new commercial launch facility. Generally, for orbital launches an ideal site would have an easterly water overflight path for safety and be located as close to the equator as possible in order to take advantage of the Earth’s rotational speed. For much of this period, a parcel of land adjacent to Boca Chica Beach near Brownsville, Texas, was the leading candidate location, during an extended period while the US Federal Aviation Administration (FAA) conducted an extensive environmental assessment on the use of the Texas location as a launch site. Also during this period, SpaceX began acquiring land in the area, purchasing approximately 41 acres (170,000 m2) and leasing 57 acres (230,000 m2) by July 2014. SpaceX announced in August 2014, that they had selected the location near Brownsville as the location for the new non-governmental launch site, after the final environmental assessment completed and environmental agreements were in place by July 2014. An orbital launch of the Starship would make it SpaceX’s fourth active launch facility, following three launch locations that are leased from the US government.

SpaceX conducted a groundbreaking ceremony on the new launch facility in September 2014, and soil preparation began in October 2015. The first tracking antenna was installed in August 2016, and the first propellant tank arrived in July 2018. In late 2018, construction ramped up considerably, and the site saw the fabrication of the first 9 m-diameter (30 ft) prototype test vehicle, Starhopper, which was tested and flown March–August 2019. Through 2021, additional prototype flight vehicles are being built at the facility for higher-altitude tests. By March 2020, there were over 500 people employed at the facility, with most of the work force involved in 24/7 production operations for the third-generation SpaceX launch vehicle, Starship.

Video credit: SpaceX

NASA dicit:

About 5,000 light-years from Earth, the stunning nebula NGC 2392 formed after the demise of a star like our Sun.

In this sonification, the image is scanned clockwise like a radar. The radius is mapped to pitch, so light farther from the center is higher pitched. The outline of the nebula’s shell can be heard in the rising and falling of pitch, punctuated by its spokes. Brightness controls the volume.

The nebula was discovered by William Herschel on January 17, 1787, in Slough, England. He described it as “A star 9th magnitude with a pretty bright middle, nebulosity equally dispersed all around. A very remarkable phenomenon. NGC 2392 WH IV-45 is included in the Astronomical League’s Herschel 400 observing program.

Video credit: NASA Goddard