Stunning new photos of the SUN show fiery plasma flowing from a honeycomb-like pattern of pores

>

Sunnycomb! Stunning new photos of the sun show hair-like strands of fiery plasma flowing from a honeycomb-like pattern of pores

  • The new images come from the Daniel K. Inouye Solar Telescope and show dramatic sunspots
  • This is the world’s most powerful ground-based solar telescope, located on the Hawaiian island of Maui

Advertisement

At first glance, you’d be forgiven for mistaking these photos as a close-up of a honeycomb-filled Crunchie chocolate bar.

But the images are actually from the world’s most powerful solar telescope and show the surface of the sun in incredible detail.

The new images come from the Daniel K. Inouye Solar Telescope and show dramatic sunspots that are larger than Earth, including one in the shape of an eerie face.

The National Science Foundation (NSF) says the scenes are a preview of the “exciting science underway” at the world’s most powerful solar telescope on the Hawaiian island of Maui.

They explain that the telescope’s unique ability to capture data in unprecedented detail will help solar scientists better understand the sun’s magnetic field and the drivers behind solar storms.

At first glance, you’d be forgiven for mistaking these photos as a close-up of a honeycomb-filled Crunchie chocolate bar. But the images are actually from the world’s most powerful solar telescope and show the surface of the sun in incredible detail

The new images come from the Daniel K. Inouye Solar Telescope and show dramatic sunspots that are larger than Earth - including one in the shape of an eerie face

The new images come from the Daniel K. Inouye Solar Telescope and show dramatic sunspots that are larger than Earth – including one in the shape of an eerie face

The National Science Foundation (NSF) says the scenes are a preview of the

The National Science Foundation (NSF) says the scenes are a preview of the “exciting science on the way” at the world’s most powerful ground-based solar telescope, which is located on the Hawaiian island of Maui.

The recently inaugurated telescope is in the Operations Commissioning Phase (OCP), a learning and transition period as the observatory is slowly being brought up to its full operational capabilities.

The new images show a variety of sunspots and quiet regions of the sun obtained by the Visible-Broadband Imager (VBI), one of the telescope’s first-generation instruments.

The sunspots pictured are dark and cool regions on the Sun’s “surface,” known as the photosphere, where strong magnetic fields are present.

The photos represent a small fraction of the data obtained from the Observation Window of Cycle 1.

The Inouye Solar Telescope data center will continue to calibrate and provide data to scientists and the public.

As the telescope continues to explore the sun, more results will come from the scientific community, including “spectacular images of our solar system’s most influential celestial body.”

The new images show a variety of sunspots and quiet regions of the sun obtained by the Visible-Broadband Imager (VBI), one of the telescope's first-generation instruments

The new images show a variety of sunspots and quiet regions of the sun obtained by the Visible-Broadband Imager (VBI), one of the telescope’s first-generation instruments

As the Inouye Solar Telescope continues to explore the sun, more results will come from the scientific community, including

As the Inouye Solar Telescope continues to explore the sun, more results will come from the scientific community, including “spectacular images of our solar system’s most influential celestial body”

This image reveals the fine structures of a sunspot in the photosphere

A detailed example of a light bridge crossing the umbra of a sunspot

The sunspots pictured are dark and cool areas on the sun’s “surface,” known as the photosphere, where strong magnetic fields persist

Sunspots vary in size, but many are often as large as Earth, if not even larger.

Complex sunspots or groups of sunspots can be the source of explosive events such as flares and coronal mass ejections that cause solar storms.

These energetic and eruptive phenomena affect the sun’s outermost atmospheric layer, the heliosphere, with the potential to affect Earth and our critical infrastructure.

In the quiet regions of the Sun, the images show convection cells in the photosphere displaying a bright pattern of hot, upward-flowing plasma (grains) surrounded by dark bands of cooler, downward-flowing solar plasma.

In the atmospheric layer above the photosphere, called the chromosphere, we see dark, elongated fibrils originating from locations of small-scale magnetic field accumulations.

The telescope's unique ability to capture data in unprecedented detail will help solar scientists better understand the sun's magnetic field and the drivers behind solar storms

The telescope’s unique ability to capture data in unprecedented detail will help solar scientists better understand the sun’s magnetic field and the drivers behind solar storms

In the atmospheric layer above the photosphere, called the chromosphere, we see dark, elongated fibrils originating from locations of small-scale magnetic field accumulations.

In the atmospheric layer above the photosphere, called the chromosphere, we see dark, elongated fibrils originating from locations of small-scale magnetic field accumulations.

The sun: the base

The sun is the star at the heart of the solar system, a near-perfect sphere of hot plasma that radiates energy.

It has a diameter of 1.39 million km and is 330,000 times the mass of the Earth.

Three quarters of the star is hydrogen, followed by helium, oxygen, carbon, neon and iron.

It is a G-type main-sequence star and is also called a yellow dwarf.

The sun was created from the gravitational collapse of matter into a large molecular cloud that gathered at its center.

The rest was flattened into a spinning disk that formed everything else.

Facts and numbers

Name: Sun

Known planets: Eight

Spectral type: G2

Distance from Earth: 150 million kilometers

Distance from galactic center: 25,800 light years

Mass: 1.9885×10^30kg

Ray: 696,342 kilometers

Brightness: 3,828×10^26W

Temperature: 9,929 F

Age: 4.6 billion years