NASA Launches SPHEREx and PUNCH to Study Sun & Universe

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What’s in Today’s Article?

NASA successfully launched the SPHEREx and PUNCH space missions from California after multiple delays.
PUNCH, a solar mission comprising four small satellites, was deployed 10 minutes after launch. It will capture detailed 3D images of the solar corona, study solar winds, and improve space weather predictions.

Spectro-Photometer for the History of the Universe, Epoch of Reionization and Ices Explorer (SPHEREx) entered a sun-synchronous orbit 650 km above Earth.
This mission will collect data from 450 million galaxies and 100 million stars to create a detailed 3D sky map and study the universe’s history.

SPHEREx will map the universe using both optical and infrared light.
While the human eye can see optical light, infrared reveals hidden details like distant galaxies, star formation, and galactic structures.
Unlike the James Webb Space Telescope (JWST), which focuses on specific regions, SPHEREx will scan the entire sky every six months in 102 infrared colors, providing an unprecedented view of the cosmos.

SPHEREx aims to shed light on cosmic inflation, a rapid expansion of the universe that occurred 14 billion years ago.
By mapping the 3D positions of 450 million galaxies, the telescope will help scientists test theories about this mysterious phenomenon, improving our understanding of the universe’s origins.

SPHEREx will search for biogenic molecules, such as carbon, hydrogen, and oxygen, frozen in icy particles across the Milky Way.
These molecules are essential for life and may have traveled to Earth from deep space.
By mapping their locations, scientists hope to uncover how these molecules contributed to the formation of life.

The Polarimetry to Unify the Corona and Heliosphere (PUNCH) mission, a solar mission comprising four small satellites, was deployed 10 minutes after launch.
It will capture detailed 3D images of the solar corona, study solar winds, and improve space weather predictions.

PUNCH is the first solar mission designed to use polarized light to measure the solar corona and solar wind in 3D.
- Polarized light consists of waves vibrating in a single plane, unlike unpolarized light, which oscillates in multiple directions.
- It occurs naturally (e.g., sky scattering) or through filters like sunglasses and scientific instruments.
The mission will provide overlapped heliospheric-coronagraphic imaging, allowing scientists to study the continuous flow of solar winds without distinct boundaries.

Solar winds and coronal mass ejections (CMEs) can disrupt satellite communications, GPS navigation, and power grids on Earth.
PUNCH’s data will enhance space weather predictions, helping protect Earth’s technology and space missions.

PUNCH consists of three Wide Field Imagers (WFI) and one Narrow Field Imager that capture images of the sun’s corona every four minutes using polarizing filters.
These images will be combined to create a detailed 3D map of the solar wind’s structure and evolution.

PUNCH will help scientists identify where solar winds and CMEs originate, how they accelerate, and their journey through interplanetary space.
This will improve timely space weather forecasting and help understand the forces acting in the corona.

Unlike previous solar missions, PUNCH’s four-camera system operates as a single virtual instrument, generating large-scale imagery data to provide an unprecedented 3D view of the sun’s outer atmosphere.