logo
Scientists say speed of Earth's rotation has increased! How will it affect our lives? Two days in July and August are important due to...

Scientists say speed of Earth's rotation has increased! How will it affect our lives? Two days in July and August are important due to...

India.com3 days ago
New Delhi: The speed of Earth's rotation on its axis is increasing. The result of the increasing speed of Earth's rotation has come in the form of a decrease in the daytime. Scientists say that it has now been confirmed that in the coming time we will see days of less than 24 hours. Scientists have said that on 22 July and 5 August, the days will be shorter by 1.3 to 1.5 milliseconds. However, the reduced duration of the day can be measured only with some special instruments. What is the usual pattern?
The general understanding about the rotation of the Earth is that the Earth revolves around the Sun in 24 hours. This is the duration of one day. This time means one day is of 24 hours. Research says that this period is not always constant. The position of the Moon and the Sun can change it with time. Even earthquakes and other geological events can change the rotation speed of the Earth. This has an effect on the time of day. What do scientists say about duration of day time?
Scientists say that the change in the time of day is not such a phenomenon that has never been seen. Days have not always been 24 hours. Researchers have found that 1 to 2 billion years ago, a day on Earth was only 19 hours long. At that time the Moon was very close to the Earth and its gravitational force was high. This distance slowed the Earth's rotation, causing the days to become longer and reach a 24-hour cycle.
After millions of years of having a 24-hour day, things have changed in recent years. Five years ago in 2020, scientists discovered that the Earth is rotating faster than at any other time in its history. In July 2024, scientists recorded a day 1.66 milliseconds less than 24 hours for the first time. This year too, scientists are saying that some days will be of less than 24-hour duration. What will be the effect on daily life?
A decrease of 1 to 2 milliseconds from the time of a day does not matter and it will not make any difference to normal life. Even our normal clocks are not able to show this difference. Experts say that this small change will also affect satellite systems, GPS and the way time is tracked.
The change in the duration of day forces international agencies like International Earth Rotation and Reference Systems Service (IERS) to adjust atomic clocks. Leap seconds have to be added or subtracted to or from them so that the official time can be synchronized with the actual rotation of the planet. Normal life remains unaffected by this.
Orange background

Try Our AI Features

Explore what Daily8 AI can do for you:

Comments

No comments yet...

Related Articles

Cosmic Baby Photo: Scientists Catch Rare First Glimpse Of Planets Being Born Around A Sun
Cosmic Baby Photo: Scientists Catch Rare First Glimpse Of Planets Being Born Around A Sun

News18

timean hour ago

  • News18

Cosmic Baby Photo: Scientists Catch Rare First Glimpse Of Planets Being Born Around A Sun

The young star, named HOPS-315, is located approximately 1,300 light-years away from Earth. It is classified as a protostar, a star in the earliest phase of development An unprecedented achievement has been made in the field of space science. For the first time, scientists have observed the earliest stages of planet formation around a newborn star similar to our Sun. This remarkable discovery was made by an international team of scientists using the James Webb Space Telescope (JWST) and the ALMA telescope. The young star, named HOPS-315, is located approximately 1,300 light-years away from Earth. It is classified as a protostar, a star in the earliest phase of development. Surrounding HOPS-315 is a protoplanetary disc made of gas and dust, which serves as the birthplace of new planets. First Signs of Planet Birth Within this disc, scientists have detected the presence of hot mineral molecules that are beginning to solidify. These minerals eventually form planetesimals, small rock-like bodies that gradually combine to become planets. Lead researcher Melissa McClure from Leiden University stated, 'This is the first time we've observed when and how planet formation begins. It offers a crucial insight into the origins of our own solar system." Co-author Merel van 't Hoff from Purdue University described the discovery as 'a childhood photo of our solar system." The key molecule identified was silicon monoxide (SiO), a mineral also found in the early rocks of Earth and other planets. These minerals, initially in gas form, are now crystallising, marking the first solid step in planet formation. Striking Similarities With Our Solar System What makes this even more intriguing is that the signals of silicon monoxide came from the same region of the disc where the asteroid belt exists in our own solar system. According to Logan Francis (Leiden University), 'We're seeing the same minerals in the same location as we do in our solar system. It's a fascinating parallel." Why HOPS-315 Is So Special The disc around HOPS-315 acts as a natural laboratory, helping us understand the early formation of solar systems. According to Elizabeth Humphreys of the European Southern Observatory (ESO), 'HOPS-315 provides a unique opportunity to study the cosmic history of our own solar system." This discovery is not just a scientific milestone; it opens a window into how worlds like ours come into being. view comments Disclaimer: Comments reflect users' views, not News18's. Please keep discussions respectful and constructive. Abusive, defamatory, or illegal comments will be removed. News18 may disable any comment at its discretion. By posting, you agree to our Terms of Use and Privacy Policy.

History made in space! Astronomers spot a solar system forming for the first time
History made in space! Astronomers spot a solar system forming for the first time

Time of India

time3 hours ago

  • Time of India

History made in space! Astronomers spot a solar system forming for the first time

For the first time, scientists have observed planets forming around a star other than our sun. Researchers used the James Webb Space Telescope and ALMA to observe planet-building material forming near the young star. This stunning discovery may help us understand how our own solar system formed 4.6 billion years ago. Explore courses from Top Institutes in Select a Course Category healthcare Digital Marketing PGDM Operations Management Artificial Intelligence Project Management Degree Cybersecurity Public Policy Finance Data Science MBA Leadership CXO Design Thinking others Management Product Management Data Analytics Technology Healthcare MCA Data Science Others Skills you'll gain: Duration: 11 Months IIM Lucknow CERT-IIML Healthcare Management India Starts on undefined Get Details Astronomers have observed the first solid materials forming around a young star known as HOPS-315 , the earliest stage of planet formation ever seen outside of our solar system. by Taboola by Taboola Sponsored Links Sponsored Links Promoted Links Promoted Links You May Like A Truck Driver's Salary in the Canada Might Surprise You Truck Driving Jobs | Search Ads Undo What makes HOPS-315 so special? The emergence of a planetary system that may eventually resemble the solar system has been observed by astronomers. The team was able to determine when the young star HOPS-315, which is about 1,300 light-years away, started to form the specks of material that will eventually form planets. Data from the Atacama Large Millimeter/submillimeter Array (ALMA), a network of 66 radio telescopes situated in the northern Chilean desert, and observations from the James Webb Space Telescope (JWST) enabled the discovery, as per a report by Space. Live Events Melissa McClure, a professor at Leiden University in the Netherlands and the study's lead author, says, "For the first time, we have identified the earliest moment when planet formation is initiated around a star other than our Sun." The study was published in Nature today. 'We're seeing a system that looks like what our Solar System looked like when it was just beginning to form," says co-author Merel van 't Hoff, a professor at Purdue University in the United States, who likens their findings to "a picture of the baby Solar System." The team's findings were released in the journal Nature on Wednesday, July 16, as per a report by ESO. ALSO READ: Massive Walmart layoffs? USA's largest private employer set to axe hundreds of jobs in shock move Around HOPS-315, a "proto" or baby star that is located about 1300 light-years away from us and is comparable to the young Sun, this newborn planetary system is beginning to form. Astronomers frequently observe "protoplanetary discs," which are discs of gas and dust that are the birthplaces of new planets, around such baby stars. But in order to observe the birth of these new "exoplanets," or extrasolar planets, astronomers had to detect protoplanetary disks earlier. How do planets begin to form around stars? Inside meteorites that have fallen to Earth, scientists can find a clue about what they should be searching for in these disks in their early stages. Meteorites are pieces of asteroids that formed during the formation of our solar system's planets 4.6 billion years ago. Meteorites, like those found in the protoplanetary disk around the sun during the early solar system, are rich in crystalline minerals that contain silicon monoxide, which condenses at high temperatures. Could this explain how Earth was born? The team found evidence of hot minerals condensing in the protoplanetary disk whirling around HOPS-315. They specifically found silicon monoxide in crystalline materials and as a gas surrounding this young star. This process has never been observed outside of our solar system or in a protoplanetary disk. ALSO READ: Who is Wilawan Emsawat? Thai woman at the heart of a shocking monk seduction and blackmail scandal Astronomers have discovered evidence that these hot minerals are starting to condense in the disc around HOPS-315. According to their findings, SiO is found both inside these crystalline minerals and surrounding the baby star in its gaseous state, indicating that it is only now starting to solidify. This process has never been observed outside of our Solar System or in a protoplanetary disc. By acting as a stand-in for young solar systems throughout the galaxy, the disc of HOPS-315 offers astronomers a fresh chance to investigate early planet formation and a fantastic analog for researching our own cosmic history. FAQs What did astronomers find near HOPS-315? They discovered early signs of solid materials, which are the basic building blocks of planets. Why is this discovery significant? It helps scientists understand how planets like Earth might have formed billions of years ago.

NASA to launch sounding rocket to study sun's chromosphere
NASA to launch sounding rocket to study sun's chromosphere

Indian Express

time4 hours ago

  • Indian Express

NASA to launch sounding rocket to study sun's chromosphere

Solar physicists will make a new attempt to observe the chromosphere of the sun, which is the most dynamic region. NASA, along with a team of international solar physicists, will launch a sounding rocket experiment on July 18 from New Mexico. Reddish in colour, the chromosphere is a region sandwiched between the sun's atmosphere (the million-degree corona) and the photosphere (the sun's visible surface). It is in the chromosphere where the solar flares, hot plasma jets, and powerful energy fluxes originate. The temperature variations recorded along this region can vary between 6000 degrees Celsius and over a million degrees Celsius. The suborbital sounding rocket experiment will last under ten minutes. On board will be the Solar EruptioN Integral Field Spectrograph (SNIFS) – a solar gazing spectrograph. a solar-gazing spectrograph solar gazing spectrograph. 'SNIFS is a first-of-its-kind solar instrument and the first ultraviolet integral field spectrograph ever flown to study the Sun. It will observe a magnetically active region on the Sun and capture high-resolution spectroscopic data from both the chromosphere and the transition region — in real time,' Souvik Bose, co-investigator of the mission, told The Indian Express. The SNIFS stands out among the heliophysics missions to study the chromosphere, as scientists will now be able to obtain a full 2D field of view, along with being able to extract a complete spectrum for every pixel in that field, thus making it a 3D data set for each moment in time. SNIFS will target the hydrogen Lyman-alpha line — the brightest line in the solar ultraviolet spectrum and one of the most powerful diagnostics for upper chromospheric conditions. 'From this, we can calculate temperatures, velocities, and densities of the solar plasma,' Bose said and further added, 'It's a dynamic, complex interface through which nearly all the energy that ultimately heats the corona must pass.' So, if we want to solve the long-standing puzzle of why the solar corona is so hot, we must first understand what is happening in the chromosphere.' The instrument comprises a Gregorian-style reflecting telescope, combined with a spectrograph via a specialised mirrorlet array that will focus on the light from each spatial location in the image. This is so that it may be spectrally dispersed without overlap from neighbouring locations. Solar physicists have noted the several challenges in observing the chromosphere and why this belt has remained elusive from detailed studies so far. Due to its composition, which is ionised plasma (a mix of charged and neutral particles), it behaves very differently in the presence of magnetic fields, and secondly, it does not adhere to the assumptions of thermodynamic equilibrium. Modelling the chromosphere has been an uphill task. But it is only an improved understanding of the chromosphere which will help scientists better understand the solar corona. The chromosphere is cooler but denser than the corona. 'This means that the chromosphere rapidly loses energy and will need a continuous supply of energy in order to stay active. Only if there is an understanding of how this energy is supplied and dissipated will it help us piece together the larger story of how the solar corona is heated,' said Bose, who is currently a research scientist at the Lockheed Martin Solar & Astrophysics Lab in California. The main agencies involved in this mission are scientists from NASA's Goddard Space Flight Center, the University of Colorado and Queen's University Belfast, UK.

DOWNLOAD THE APP

Get Started Now: Download the App

Ready to dive into a world of global content with local flavor? Download Daily8 app today from your preferred app store and start exploring.
app-storeplay-store