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Subject: Space Technology

  • CHIME Telescope

    Scientists with the Canadian Hydrogen Intensity Mapping Experiment (CHIME) Collaboration have assembled the largest collection of fast radio bursts (FRBs) in the telescope’s first FRB catalog.

    CHIME Telescope

    • CHIME is an interferometric radio telescope at the Dominion Radio Astrophysical Observatory in British Columbia, Canada.
    • It consists of four antennas consisting of 100 x 20-meter cylindrical parabolic reflectors with 1024 dual-polarization radio receivers suspended on support above them.
    • The telescope receives radio signals each day from half of the sky as the Earth rotates.
    • While most radio astronomy is done by swiveling a large dish to focus light from different parts of the sky, CHIME stares, motionless, at the sky, and focuses incoming signals using a correlator.
    • This is a powerful digital signal processor that can work through huge amounts of data, at a rate of about seven terrabytes per second, equivalent to a few percent of the world’s Internet traffic.

    What are FRBs?

    • FRBs are oddly bright flashes of light, registering in the radio band of the electromagnetic spectrum, which blaze for a few milliseconds before vanishing without a trace.
    • These brief and mysterious beacons have been spotted in various and distant parts of the universe, as well as in our own galaxy.
    • Their origins are unknown and their appearance is highly unpredictable.
    • But the advent of the CHIME project has nearly quadrupled the number of fast radio bursts discovered to date.
    • With more observations, astronomers hope soon to pin down the extreme origins of these curiously bright signals.
  • CIBER-2 Mission to count the stars in the Universe

    A NASA-funded rocket’s launch window will open at the White Sands Missile Range in New Mexico, USA. The aim of this mission is to count the number of stars that exist in the Universe.

    Answer this PYQ from CSP 2020 in the comment box:

    Q.“The experiment will employ a trio of spacecraft flying in formation in the shape of an equilateral triangle that has sides one million kilometers long, with lasers shining between the craft.” The experiment in question refers to

    (a) Voyager-2

    (b) New horizons

    (c) Lisa Pathfinder

    (d) Evolved LISA

    What is CIBER-2?

    • In order to roughly estimate the number of stars in the Universe, scientists have estimated that on average each galaxy consists of about 100 million stars, but this figure is not exact.
    • The figure of 100 million could easily be an underestimation, probably by a factor of 10 or more.
    • To put this into perspective, an average of 100 million stars in each galaxy (there an estimated 2 trillion of them as per NASA), would give a total figure of one hundred quintillion stars or 1 with 21 zeroes after it.
    • NASA notes that if this figure is accurate, it would mean that for every grain of sand on Earth, there are more than ten stars.
    • But this calculation assumes that all stars are inside galaxies, which might not be true and this is what the CIBER-2 instrument will try to find out.

    How will CIBER-2 count stars?

    • NASA notes that the instrument will not actually count individual stars but it will instead detect the extragalactic background light
    • It is all of the light that has been emitted throughout the history of the Universe.
    • From all of this extragalactic background light, the CIBER-2 will focus on a portion of this called cosmic infrared background, which is emitted by some of the most common stars.
    • Essentially, this approach is aiming to look at how bright this light is to give scientists an estimate of how many of these stars are out there.
    • The ESA infrared space observatory Herschel also counted the number of galaxies in infrared and measured their luminosity previously.
  • DAVINCI+ and VERITAS missions for exploration of Venus

    NASA has selected two missions to the planet Venus, Earth’s nearest neighbor. The missions are called DAVINCI+ and VERITAS.

    DAVINCI+ and VERITAS

    (1) DAVINCI+

    • DAVINCI+ is short for ‘Deep Atmosphere Venus Investigation of Noble gases, Chemistry, and Imaging’ and is the first US-led mission to the planet’s atmosphere since 1978.
    • It will try to understand Venus’ composition to see how the planet formed and evolved.
    • This mission also consists of a decent sphere that will pass through the planet’s thick atmosphere and make observations and take measurements of noble gases and other elements.
    • Significantly, this mission will also try to return the first high-resolution photographs of a geological feature that is unique to Venus.
    • This feature, which is called “tesserae” may be comparable to Earth’s continents.
    • The presence of tesseraes may suggest that Venus has tectonic plates like Earth.

    (2) VERITAS

    • The second mission called VERITAS is short for ‘Venus Emissivity, Radio Science, InSAR, Topography, and Spectroscopy’.
    • It will map the planet’s surface to determine its geologic history and understand the reasons why it developed so differently from Earth.
    • VERITAS will orbit Venus with a radar that will help to create a 3D reconstruction of its topography which might be able to tell scientists if processes such as plate tectonics and volcanism are still active there.
    • This mission will also map the emissions from Venus’s surface that may help in determining the type of rocks that exist on Venus–a piece of information that is not exactly known yet.
    • It will also determine if active volcanoes are releasing water vapor into the atmosphere.

    Why study Venus?

    • The results from DAVINCI+ are expected to reshape the understanding of terrestrial planet formation in the solar system and beyond.
    • Taken together, both missions are expected to tell scientists more about the planet’s thick cloud cover and the volcanoes on its surface.
    • Further, scientists speculate about the existence of life on Venus in its distant past and the possibility that life may exist in the top layers of its clouds where temperatures are less extreme.

    Have humans visited Venus?

    • Because of the planet’s harsh environment, no humans have visited it and even the spacecraft that have been sent to the planet have not survived for a very long time.
    • Venus’ high surface temperatures overheat electronics in spacecraft in a short time, so it seems unlikely that a person could survive for long on the Venusian surface.
    • So far, spacecraft from several nations have visited the planet.
    • The first such spacecraft was the Soviet Union’s Venera series (the spacecraft, however, could not survive for long because of the planet’s harsh conditions).
    • It was followed by NASA’s Magellan Mission that studied Venus from 1990-1994. As of now, Japan’s Akatsuki mission is studying the planet from Orbit.

    Back2Basics: Venus

    • For those on Earth, Venus is the second-brightest object in the sky after the moon.
    • It appears bright because of its thick cloud cover that reflects and scatters light.
    • Surface temperatures on Venus can go up to 471 degrees Celsius, which is hot enough to melt lead, NASA notes. Surface temperatures on Venus can go up to 471 degrees Celsius, which is hot enough to melt lead, NASA notes.

    Some unknown facts

    • While Venus, which is the second closest planet to the Sun, is called the Earth’s twin because of their similar sizes, the two planets have significant differences between them.
    • For one, the planet’s thick atmosphere traps heat and is the reason that it is the hottest planet in the solar system, despite coming after Mercury, the closest planet to the Sun.
    • Further, Venus moves forward on its orbit around the Sun but spins backwards around its axis slowly.
    • This means on Venus the Sun rises in the west and sets in the East.
    • One day on Venus is equivalent to 243 Earth days because of its backward spinning, opposite to that of the Earth’s and most other planets.
    • Venus also does not have a moon and no rings.
  • OneWeb constellation for Internet from the Skies

    Following the successful launch of 36 satellites, OneWeb’s Low Earth Orbit (LEO) constellation reached 218 in-orbit satellites.

    What is OneWeb?

    • OneWeb is a global communications company that aims to deliver broadband satellite Internet around the world through its fleet of LEO satellites.
    • OneWeb satellites are built at a OneWeb and Airbus joint venture facility in Florida that can produce up to two satellites a day.
    • The launch roll-out of the satellites is facilitated by French company Arianespace using Russian-made Soyuz rockets.
    • The company has announced plans to enter the Indian market by 2022.

    About its constellation

    • The company has one more launch to complete before it obtains the capacity to enable its ‘Five to 50’ service of offering internet connectivity to all regions north of 50 degrees latitude.
    • The Five to 50 service is expected to be switched on by June 2021 with global services powered by 648 satellites available in 2022.

    What are LEO satellites?

    • LEO satellites have been orbiting the planet since the 1990s, providing companies and individuals with various communication services.
    • They are positioned around 500km-2000km from earth, compared to stationary orbit satellites which are approximately 36,000km away.
    • Latency, or the time needed for data to be sent and received, is contingent on proximity.
    • As LEO satellites orbit closer to the earth, they are able to provide stronger signals and faster speeds than traditional fixed-satellite systems.
    • Additionally, because signals travel faster through space than through fiber-optic cables, they also have the potential to rival if not exceed existing ground-based networks.
    • However, LEO satellites travel at a speed of 27,000 kph and complete a full circuit of the planet in 90-120 minutes.
    • As a result, individual satellites can only make direct contact with a land transmitter for a short period of time thus requiring massive LEO satellite fleets and consequently, a significant capital investment.

    Criticisms of LEO satellites

    • During the days of the Sputnik and Apollo missions, governments dominated and regulated space-based activities.
    • There are logistical challenges with launching thousands of satellites into space as well.
    • Satellites can sometimes be seen in the night skies which creates difficulties for astronomers as the satellites reflect sunlight to earth, leaving streaks across images.
    • Satellites traveling at a lower orbit can also interrupt the frequency of those orbiting above them, an accusation that has been leveled against Starlink satellites already.
    • Another worry is that there are already almost 1 million objects larger than 1cm in diameter in orbit, a byproduct of decades of space activities.
    • Those objects, colloquially referred to as ‘space junk,’ have the potential to damage spacecraft or collide with other satellites.
  • [pib] 3D distribution of Molecular & Atomic Hydrogen in Galaxies

    Indian scientists have estimated the three-dimensional distribution of molecular and atomic hydrogen in a nearby galaxy which can help lead to clues to the star formation processes and the evolution of the galaxy.

    Study on Hydrogen distribution

    • Galaxies like the one we reside in, the Milky Way, consist of discs containing stars, molecular and atomic hydrogen, and helium.
    • The molecular hydrogen gas collapses on itself in distinct pockets, forming stars, its temperature was found to be low –close to 10 kelvin, or -263 ºC, and thickness is about 60 to 240 light-years.
    • The atomic hydrogen extends both above and below the discs.
    • Indian scientists have estimated that molecular hydrogen extends farther from the disc in both directions, up to about 3000 light-years.
    • This gaseous component is warmer than the one straddling the disc and has comparatively lesser densities, thus escaping earlier observations.
    • They called it the ‘diffuse’ component of the molecular disc.

    Answer this PYQ in the comment box:

    Q. Which one of the following sets of elements was primarily responsible for the origin of life on the Earth?

    (a) Hydrogen, Oxygen, Sodium

    (b) Carbon, Hydrogen, Nitrogen

    (c) Oxygen, Calcium, Phosphorous

    (d) Carbon, Hydrogen, Potassium

    Why does this study matter?

    • The molecular hydrogen gas converts to individual stars under the pull of gravity, thus holding clues to the star formation processes and the evolution of the galaxy.
    • If a significant part of the gas extends beyond the thin disc of a few hundred light-years, it may explain why astronomers also observe stars at a few thousand light-years perpendicular to the galactic disc.
  • Tianwen-1 lands successfully on Mars

    China landed a spacecraft on Mars carrying its first Mars rover in a big boost to its space ambitions.

    UPSC may ask an MCQ asking: Which of the following is/are the space missions related to Mars? It may throw up 4-5 options (which we all get confused at after few months) like Cassini , InSight , Messanger, Voyager etc.

    Tianwen-1 Mission

    • The mission is named after the ancient Chinese poem ‘Questions to Heaven’, the Tianwen-1.
    • It is an all-in-one orbiter; lander and rover will search the Martian surface for water, ice, investigate soil characteristics, and study the atmosphere, among completing other objectives.
    • It will be the first to place ground-penetrating radar on the Martian surface, which will be able to study local geology, as well as rock, ice, and dirt distribution.
    • The lander descended successfully onto the surface of the red planet carrying a rover named Zhurong, named after a god of fire for a planet known in Chinese as the planet of fire.
    • Only the Soviet Union and the United States had previously carried out a successful landing on Mars.

    Back2Basics: Various missions on Mars

    • The USSR in 1971 became the first country to carry out a Mars landing– its ‘Mars 3’ lander being able to transmit data for 20 seconds from the Martian surface before failing.
    • The country made it’s second and Mars landing two years later in 1973.
    • The second country to reach Mars’s surface, the US, holds the record for the most number of Mars landings.
    • Since 1976, it has achieved 8 successful Mars landings, the latest being the ‘InSight’ in 2019 (launched in 2018).
    • India and the European Space Agency have been able to place their spacecraft in Mars’s orbit.
    • India’s Mars Orbiter Mission (MOM) or ‘Mangalyaan’ was able to do so in September 2014, almost a year after its launch from the Satish Dhawan Space Centre in Andhra Pradesh.
    • The Chinese mission now is expected to take off around the same time when NASA is launching its own Mars mission– the ambitious ‘Perseverance’ which aims to collect Martian samples and bring them back.
  • NASA’s OSIRIS-REx begins journey back from asteroid

    On May 11, NASA’s Origins, Spectral Interpretation, Resource Identification, Security, Regolith Explorer (OSIRIS-REx) spacecraft will depart asteroid Bennu, and start its two-year-long journey back to Earth.

    About OSIRIS-REx

    • OSIRIS-REx is NASA’s first mission to visit a near-Earth asteroid, survey its surface and collect a sample from it.
    • The mission was launched in 2016, it reached its target in 2018 and since then, the spacecraft has been trying to match the velocity of the asteroid using small rocket thrusters.
    • It also utilised this time to survey the surface and identify potential sites to take samples.
    • In October 2020, the spacecraft briefly touched asteroid Bennu, from where it collected samples of dust and pebbles. 
    • Once the surface was disturbed, the spacecraft’s robotic arm captured some samples.
    • The spacecraft’s engineers have also confirmed that shortly after the spacecraft made contact with the surface, it fired its thrusters and “safely backed away from Bennu”.

    About Bennu

    • Bennu is considered to be an ancient asteroid that has not gone through a lot of composition-altering change through billions of years, which means that below its surface lie chemicals and rocks from the birth of the solar system.
    • Around 20-40 percent of Bennu’s interior is empty space and scientists believe that it was formed in the first 10 million years of the solar system’s creation, implying that it is roughly 4.5 billion years old.
    • Bennu is a B-type asteroid, implying that it contains significant amounts of carbon and various other minerals.
    • Because of its high carbon content, the asteroid reflects about four percent of the light that hits it, which is very low when compared with a planet.
    • Bennu is named after an Egyptian deity.
    • The asteroid was discovered by a team from the NASA-funded Lincoln Near-Earth Asteroid Research team in 1999.
  • [pib] Narrow-Line Seyfert 1 (NLS1) Galaxy

    Astronomers have discovered a new active galaxy identified as the farthest gamma-ray emitting galaxy that has so far been stumbled upon. This active galaxy called the Narrow-Line Seyfert 1 (NLS1) galaxy.

    Try this PYQ:

    Q.Recently, scientists observed the merger of giant ‘blackholes’ billions of light-years away from the Earth. What is the significance of this observation?

    (a) ‘Higgs boson particles’ were detected.

    (b) ‘Gravitational waves’ were detected.

    (c) Possibility of inter-galactic space travel through ‘wormhole’ was confirmed.

    (d) It enabled scientists to understand ‘singularity’.

    NLS1 Galaxy

    • Indian scientists have studied around 25,000 luminous Active galactic nuclei (AGN) from the Sloan Digital Sky Survey (SDSS).
    • They identified it as a gamma-ray emitting NLS1 galaxy, which is a rare entity in space.
    • It is about 31 billion light-years away, opens up avenues to explore more such gamma-ray emitting galaxies that wait to meet us.

    What makes it intriguing?

    • Ever since 1929, when Edwin Hubble discovered that the Universe is expanding, it has been known that most other galaxies are moving away from us.
    • Light from these galaxies is shifted to longer (and this means redder) wavelengths – in other words, it is red-shifted.
    • Scientists have been trying to trace such red-shifted galaxies to understand the early Universe.
    • Powerful relativistic jets, or sources of particles in the Universe travelling nearly at speed to light, are usually produced by AGN powered by large black holes and hosted in a giant elliptical galaxy.

    Why NLS1 is unique?

    • NLS1s are a unique class of AGN that are powered by the black hole of low mass and hosted in a spiral galaxy.
    • As of today, gamma-ray emission has been detected in about a dozen NLS1 galaxies, which are a separate class of AGN identified four decades ago.
    • All of them are at redshifts lesser than one, and no method was present to date to find NLS1 at redshifts larger than one.
    • This discovery opens up a new way to find gamma-ray emitting NLS1 galaxies in the early Universe.
  • [pib] What are Wolf–Rayet Stars?

    Indian astronomers have tracked a rare supernova explosion and traced it to one of the hottest kind of stars called Wolf–Rayet stars or WR stars.

    Space science-related terms these days are often focused on Gravitational waves, Black holes etc. But basic terminologies are very important and need to be taken care of. For example, a layman may hardly find any difference between Novae-Supernovae, Neutron star, Nebula etc. UPSC often tries to bust you with such basic differences.

    Wolf–Rayet Stars

    • Wolf-Rayet stars represent a final burst of activity before a huge star begins to die.
    • These stars, which are at least 20 times more massive than the Sun, “live fast and die hard”.
    • Wolf-Rayets stars are divided into 3 classes based on their spectra, the WN stars (nitrogen dominant, some carbon), WC stars (carbon dominant, no nitrogen) and WO where oxygen is in dominant quantities.
    • The average temperature of a Wolf-Rayet star is greater than 25,000 Kelvin, and they can have luminosities of up to a million times that of the Sun.

    What have Indian researchers studied?

    • Indian astronomers have conducted the optical monitoring of one such stripped-envelope supernova called SN 2015dj hosted in the galaxy NGC 7371 which was spotted in 2015.
    • They calculated the mass of the star that collapsed to form the supernovae as well as the geometry of its ejection.

    Their findings

    • The scientists found that the original star was a combination of two stars – one of them is a massive WR star and another is a star much less in mass than the Sun.
    • Supernovae (SNe) are highly energetic explosions in the Universe releasing an enormous amount of energy.
    • Long-term monitoring of these transients opens the door to understand the nature of the exploding star as well as the explosion properties.
    • It can also help enumerate the number of massive stars.
  • Martian ‘Blueberries’

    In 2004, NASA’s Mars exploration rover ‘Opportunity’ found several small spheres on the planet, informally named Martian blueberries which find a resemblance to the similar formation in India’s Kutch region.

    There have been several missions to the red planet this year. Make a note of all of them.

    Martian blueberries

    • Opportunity’s mini spectrometers studied mineralogy and noted they were made of iron oxide compounds called haematites.
    • This caused excitement, as the presence of haematites suggests that there was water present on Mars.
    • The widely accepted formation mechanism of hematite concretion [hard solid mass] is precipitation from aqueous fluids.
    • Hematite is known to form in oxidizing environments hence it can be inferred that water must have played a crucial role in the formation of grey hematite on Mars.

    What makes them so special?

    • Indian researchers have been studying hematite concretions in Kutch called the Jhuran formation.
    • These formations are 145 and 201 million years old.
    • Detailed geochemistry and spectroscopic investigations of the haematite concretions in this area revealed that they resemble the ones on Mars.
    • They have similar morphology – spherical, often doublet and triplet – and similar mineralogy – a mixture of haematite and goethite.
    • Hence, several types of research have shown that the Kutch area is a potential Martian analogue locality.