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Fish Fibroblast

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Honorable Mention: CAR Fish Fibroblast

Maria Nemethova, IMBA - Institute of Molecular Biotechnology GmbH, Vienna, Austria
Subject: CAR fish fibroblast transfected with mCherry-Actin and GFP-Vasp
Magnification: 100x
Technique: Epifluorescence

This video illustrates the polymerization of actin, a protein which drives cell movements. Actin acts like the “scaffold” of a cell, so understanding how it forms is important is to basic cellular research and can help answer further questions on how cells form.


Microtubule Asters

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Honorable Mention: Microtubule Asters Recapitulated in a Model Cytoplasm

Phuong Anh Nguyen, Harvard Medical School, Boston, Massachusetts
Subject: Time lapse movie of microtubule asters growing in a thin layer of interphase Xenopus (frog) egg extract
Magnification: 10x
Technique: Widefield Fluorescence Microscopy

This movie shows the growth, interaction, and movement of microtubule asters (in green) in Xenopus (frog) egg cytoplasm, following exit from metaphase (cell division). Asters grown in a thin layer of cytoplasm between two glass coverslips recapitulates the behavior of asters in early dividing live embryos during anaphase/telophase/cytokinesis. Where asters meet, cytokinesis proteins such as the chromosomal passenger complex (visualized using a fluorescently labeled antibody against a CPC component, shown in red) are recruited. This establishes a boundary between the two asters, and marks the position of the putative cleavage furrow.

Onion Bulb Scale Epidermis

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Honorable Mention: Onion Bulb Scale Epidermis

Heiti Paves, Tallinn University of Technology, Tallinn, Estonia
Subject: Movement of organelles in plant cells (onion bulb scale epidermis)
Magnification: 20x
Technique: Differential Interference Contrast

This video captures the continuous movement of organelles in plant cells without any obvious reason, captured with a laser scanning confocal microscope with a regular SLR camera to get enough speed.

Arabidopsis endosomes

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Honorable Mention: Arabidopsis endosomes

Daniel von Wangenheim, Goethe University Frankfurt, Frankfurt am Main, Hessen, Germany
Subject: Fast moving endosomes in Arabidopsis thaliana root cells
Magnification: 63x
Technique: Light Sheet-based Fluorescence Microscopy

A sheet of light is used to illuminate the plant (Arabidopsis thaliana), from the side while collecting the emitted light at a perpendicular axis. The plant grows in an upright position in the microscope’s specimen chamber. While the leaves remain in the air, the root system is perfused with liquid medium. and root stably expresses the early endosome/exosome marker 35S::GFP-RabA1d. The quick endosomes move with up to 10 µm/s, which presents a serious imaging challenge. This technique allows new insides in the dynamics of endosomal compartments in plant cells. The Arabidopsis line was kindly provided by Tobias Berson and Jozef Samaj.

Action of the Heart

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Honorable Mention: Action of the Heart

Michael Weber, Max Planck Institute of Molecular Cell Biology and Genetics, Dresden, Germany
Subject: Beating heart of a living 2-day-old Danio rerio (zebrafish)
Magnification: 20x
Technique: Selective Plane Illumination Microscopy (SPIM)

The heart muscle cells of this transgenic fish expresses GCaMP, a genetically encoded fluorescent calcium indicator. Visible is the wave of cardiac conduction, traveling over the heart from atrium (bottom) to ventricle (top left). The heart has a size of about 250 um and beats at a rate of about two times per second. It was imaged in 3D inside the living zebrafish using Selective Plane Illumination Microscopy (SPIM) (Huisken et al. 2004).

The Making of the Brain

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Honorable Mention: The Making of the Brain

Fengzhu Xiong, Harvard Medical School, Boston, Massachusetts
Subject: Imaging of the formation of the anterior hindbrain from a flat sheet of neural plate cells in a zebrafish embryo
Magnification: 400x
Technique: Confocal Timelapse

The video demonstrates the formation of the anterior hindbrain from a flat sheet of neural plate cells in a zebrafish embryo. In particular, we view the patterns of the nervous system, which are important for understanding human disease. Membrane and nuclear fluorescent proteins were used to label the cells.

Jan 17, 2013

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Moody, Glowing Saturn Auroras

This false-color composite image, constructed from data obtained by NASA's Cassini spacecraft, shows the glow of auroras streaking out about 1,000 km (600 miles) from the cloud tops of Saturn's south polar region. It is among the first images released from a study that identifies images showing auroral emissions out of the entire catalogue of images taken by Cassini's visual and infrared mapping spectrometer.

In this image constructed from data collected in the near-infrared wavelengths of light, the auroral emission is shown in green. The data represents emissions from hydrogen ions in of light between 3 and 4 microns in wavelength. In general, scientists designated blue to indicate sunlight reflected at a wavelength of 2 microns, green to indicate sunlight reflected at 3 microns and red to indicate thermal emission at 5 microns. Saturn's rings reflect sunlight at 2 microns, but not at 3 and 5 microns, so they appear deep blue. Saturn's high altitude haze reflects sunlight at both 2 and 3 microns, but not at 5 microns, and so it appears green to blue-green. The heat emission from the interior of Saturn is only seen at 5 microns wavelength in the spectrometer data, and thus appears red. The dark spots and banded features in the image are clouds and small storms that outline the deeper weather systems and circulation patterns of the planet. They are illuminated from underneath by Saturn's thermal emission, and thus appear in silhouette.

The composite image was made from 65 individual observations by Cassini's visual and infrared mapping spectrometer on 1 November 2008. The observations were each six minutes long.

Image: NASA/JPL/University of Arizona/University of Leicester [high-resolution]

Caption: Cassini Solstice team

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Europa’s Broken Surface

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Europa’s Broken Surface

Scientists suspect that Jupiter’s moon Europa contains a gigantic hidden ocean beneath its icy outer shell. The finding suggests that the moon possesses some sort of tectonic mechanism for generating heat, melting its ice, and creating the ocean. This image, from the Galileo spacecraft in 1996, shows cracks and pits peppering Europa’s surface.

Image: NASA/JPL/University of Arizona/University of Colorado

First Mars Image

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First Mars Image

One of the earliest images from Mars comes from this strange picture from the Mariner 4 mission in 1964. Too anxious to wait for the official processed shot from the spacecraft, engineers at JPL simply converted the image data into integers and then hand colored it in like a paint-by-numbers drawing.

Mariner 4 transmitted the first close-up pictures of another planet to Earth and revealed Mars to be a dry, desert-like world very unlike our own.

Image: NASA/JPL/Dan Goods

Iapetus’ Ridge

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Iapetus’ Ridge

Saturn’s moon Iapetus has an incredible and unique geologic feature, a ridge 20 km high that runs for 1,300 km along the moon’s equator.

Image: NASA/JPL/Space Science Institute

Volcanic Io

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Volcanic Io

When NASA’s Voyager 1 mission zipped by the Jupiter system in 1979, it discovered that far from the sun were worlds of unimaginable activity. In particular, it shot spectacular pictures of the moon Io, which was covered in volcanoes and is now known to be one of the most geologically active places in the solar system. This image shows a plume from a volcano on Io’s surface.

Image: NASA/JPL

Miranda’s Chevrons

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Miranda’s Chevrons

Uranus’ moon Miranda is a jumbled assemblage of older, heavily cratered terrain, interspersed with young land covered in scarps and ridges. One of Miranda’s distinctive “chevron” features, a v-shaped landscape. This image comes from Voyager 2.

Image: NASA/JPL/USGS

What Makes Up the Moon

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Before 1962, most of the planets in our solar system were hardly more than blurry dots in some astronomer’s telescope.

The most the scientists knew about Mercury, Venus, or Jupiter was their size, surface temperature, and atmospheric composition. But on Dec. 14 of that year, the Mariner 2 spacecraft flew by Venus. For the first time, researchers had detailed and up-close information about other worlds, helping spawn new fields such as astrogeology and modern planetary science. The planets in our solar system changed from distant points to fully-fledged worlds, with distinctive and amazing features.

Image: A roll of data from Venus from the 1962 Mariner 2 mission. NASA

A recent issue of Eos, the weekly magazine published by the American Geophysical Union, praised the last 50 years of solar system exploration in a special feature. The article highlighted how much knowledge scientists have gained in the half-century since Mariner 2’s flight and reminded readers of the unique time we are living in.

“As Carl Sagan used to say, only one generation of humankind can be the first explorers of the solar system, and we are that generation,” wrote astrogeologist Michael Carr from the U.S. Geological Survey (USGS) in the feature.

Here we take a look at just one small sliver from the wealth of information that has come to us from five decades of robotic spaceflight. In this gallery, we can see how our knowledge has grown in leaps and bounds during the last 50 years by looking at some of the biggest, most impressive, and all around greatest geologic structures in the solar system.

Above:

What Makes Up the Moon

In 1992, the Jupiter-bound Galileo spacecraft made a pass by our planet’s closest companion, the moon. This mosaic shows the different composition of rocks left behind by lava flows early in the moon’s history.

Image: NASA/JPL


Olympus Mons

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Olympus Mons

The biggest mountain in the solar system is Olympus Mons, towering at nearly 22 km, or more than three times the height of Mount Everest on Earth. It’s entire expanse takes up the same area as some medium-sized countries.

Image: NASA/MOLA Science Team/ O. de Goursac, Adrian Lark

South-Pole Aiken Basin

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South-Pole Aiken Basin

One of largest impact craters in the solar system is the lunar South Pole Aiken Basin. Located on the far side of the moon (which never faces the Earth) it was only possible to discover this feature with robotic probes. Since the mid-1960s, scientists have recognized its enormous dimensions: roughly 2,500 km across, while the moon itself is only 3,500 km in diameter to begin with.

The image above comes from the Lunar Reconnaissance Orbiter, one of NASA’s most recent missions. It contrasts well with the first image of the moon taken by a U.S. spacecraft — the Ranger 7 mission of 1964 – which shows several craters. The large crater in the center right is called Alphonsus, flanked above by Ptolemaeus and below by Arzachel.

Images: 1) NASA/Goddard 2) NASA/JPL

Triton’s Volcanoes

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Triton’s Volcanoes

To find a volcanically active place at the furthest reaches of the solar system was certainly a surprise when scientists got their first glimpse of Neptune’s moon Triton with the Voyager 2 spacecraft in 1989. But the moon’s surface is young, possibly younger than Europa’s, perhaps the result of internal heating. This view shows a volcanic plain on the moon.

Image: NASA/JPL/Universities Space Research Association/Lunar & Planetary Institute

Aphrodite Terra

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Aphrodite Terra

Aphrodite is an enormous continent on the surface of Venus. This image, from the Magellan spacecraft taken in 1991, features this bright region in its center. Venus is known to have been an extremely volcanically active planet throughout its history, though whether or not there is still any active tectonics remains a mystery.

Image: NASA/JPL

Jan 22, 2013

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Stephan's Quintet

This grouping of five galaxies 280 million light-years away in the constellation Pegasus is known as Stephan's Quintet. Four of the five galaxies are experiencing a violent merger, where they crash into one another an eventually form one galaxy. Though it looks like the central blue galaxy is part of this clan, this is an illusion. It is actually a foreground galaxy only about 40 million light-years away.

This image, from the Arizona Sky Center, required a 5-hour exposure using the 32-inch Schulman telescope.

Image: Adam Block and Vic Eden/Mount Lemmon SkyCenter/University of Arizona [high-resolution]

Caption: Wired Science

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