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authorZachary Betz <zwbetz@gmail.com>2018-12-28 07:40:33 +0300
committerZachary Betz <zwbetz@gmail.com>2018-12-28 07:40:33 +0300
commit962b255e462399adcb20fe9dbbf3a5a6dad09c7f (patch)
tree9a2b0270d464cfc8c7944cf8e15e68de68085129
parent279191474c706a64c2d73422476d502b0958c9c2 (diff)
Shorten card text
-rw-r--r--exampleSite/content/post/nasa-images/index.md6
1 files changed, 3 insertions, 3 deletions
diff --git a/exampleSite/content/post/nasa-images/index.md b/exampleSite/content/post/nasa-images/index.md
index 8036f79..b50bcd5 100644
--- a/exampleSite/content/post/nasa-images/index.md
+++ b/exampleSite/content/post/nasa-images/index.md
@@ -9,7 +9,7 @@ Images from the [NASA Image and Video Library](https://images.nasa.gov/).
{{< bootstrap-card
img="sun.jpg"
title="The Sun"
-text="This illustration lays a depiction of the sun's magnetic fields over an image captured by NASA’s Solar Dynamics Observatory on March 12, 2016. The complex overlay of lines can teach scientists about the ways the sun's magnetism changes in response to the constant movement on and inside the sun. Note how the magnetic fields are densest near the bright spots visible on the sun – which are magnetically strong active regions – and many of the field lines link one active region to another. This magnetic map was created using the PFSS – Potential Field Source Surface – model, a model of the magnetic field in the sun’s atmosphere based on magnetic measurements of the solar surface. The underlying image was taken in extreme ultraviolet wavelengths of 171 angstroms. This type of light is invisible to our eyes, but is colorized here in gold. [Credits](https://images.nasa.gov/details-GSFC_20171208_Archive_e000393.html)."
+text="The Sun is the star at the center of the Solar System. It is a nearly perfect sphere of hot plasma, with internal convective motion that generates a magnetic field via a dynamo process. It is by far the most important source of energy for life on Earth. [Credits](https://images.nasa.gov/details-GSFC_20171208_Archive_e000393.html)."
alt="sun"
command="Resize"
options="700x"
@@ -18,7 +18,7 @@ class="mb-3" >}}
{{< bootstrap-card
img="moon.jpg"
title="The Moon"
-text="Full Moon. Rises at sunset, high in the sky around midnight. Visible all night. This marks the first time that accurate shadows at this level of detail are possible in such a computer simulation. The shadows are based on the global elevation map being developed from measurements by the Lunar Orbiter Laser Altimeter (LOLA) aboard the Lunar Reconnaissance Orbiter (LRO). LOLA has already taken more than 10 times as many elevation measurements as all previous missions combined. The Moon always keeps the same face to us, but not exactly the same face. Because of the tilt and shape of its orbit, we see the Moon from slightly different angles over the course of a month. When a month is compressed into 12 seconds, as it is in this animation, our changing view of the Moon makes it look like it's wobbling. This wobble is called libration. The word comes from the Latin for \"balance scale\" (as does the name of the zodiac constellation Libra) and refers to the way such a scale tips up and down on alternating sides. [Credits](https://images.nasa.gov/details-GSFC_20171208_Archive_e001861.html)."
+text="The Moon is an astronomical body that orbits planet Earth and is Earth's only permanent natural satellite. It is the fifth-largest natural satellite in the Solar System, and the largest among planetary satellites relative to the size of the planet that it orbits (its primary). The Moon is after Jupiter's satellite Io the second-densest satellite in the Solar System among those whose densities are known. [Credits](https://images.nasa.gov/details-GSFC_20171208_Archive_e001861.html)."
alt="moon"
command="Resize"
options="700x"
@@ -27,7 +27,7 @@ class="mb-3" >}}
{{< bootstrap-card
img="earth.jpg"
title="The Earth"
-text="Behold one of the more detailed images of the Earth yet created. This Blue Marble Earth montage shown above -- created from photographs taken by the Visible/Infrared Imager Radiometer Suite (VIIRS) instrument on board the new Suomi NPP satellite -- shows many stunning details of our home planet. The Suomi NPP satellite was launched last October and renamed last week after Verner Suomi, commonly deemed the father of satellite meteorology. The composite was created from the data collected during four orbits of the robotic satellite taken earlier this month and digitally projected onto the globe. Many features of North America and the Western Hemisphere are particularly visible on a high resolution version of the image. [Credits](https://images.nasa.gov/details-PIA18033.html)."
+text="Earth is the third planet from the Sun and the only astronomical object known to harbor life. According to radiometric dating and other sources of evidence, Earth formed over 4.5 billion years ago. Earth's gravity interacts with other objects in space, especially the Sun and the Moon, Earth's only natural satellite. Earth revolves around the Sun in 365.26 days, a period known as an Earth year. During this time, Earth rotates about its axis about 366.26 times. [Credits](https://images.nasa.gov/details-PIA18033.html)."
alt="earth"
command="Resize"
options="700x"