Life aboard the SS Great Britain

THE SOAR SYSTEM A solar system is a group of planets and other celestial bodies that revolve around a star. A solar nebula- a vast cloud of gas and dust, mostly hydrogen and helium. How the Solar System Form • COLLAPSE AND SPINNING DISK FORMATION - Gravity pulls material inward. The cloud flattens into a spinning disk due to conservation of angular momentum. • PROTOSTAR FORMATION- (BIRTH OF THE SUN). Material collects at the center, and begun to heat up. When it reaches to 10 million KELVIN, nuclear fusion begins. thus, SUN is born. • PLANETESIMALS AND PROTOPLANETS. Dust and gas in the disk stick together via static and gravitational forces. These form planetesimals, which grow into protoplanets collision and accretion. • PLANET FORMATION. Inner disk: too hot for gas rocky planets form Mercury, Venus, Earth, Mars. • PLANET FORMATION. Outer disk: gas and ice giants. Jupiter, Saturn, Uranus, Neptune • LEFTOVER DEBRIS. Remaining materials forms moon, asteroids, comets and dwarf planets. DIFFERENT HYPOTHESIS IN THE FORMATION OF SOLAR SYSTEM. 1. NEBULAR HYPOTHESIS- The Solar system formed from a rotating cloud of Gas and Dust (solar nebula). As it rotates conservation of angular momentum caused the cloud to flatten into a disk. the Sun formed at the center (DISK) while planets formed from the surrounding materials through acceleration. thus, it explains the coplanar and nearly circular orbit of the planets all planets orbits around the sun on the same flat, disk shaped plane. Proposed by Immanuel Kant in 1755 and Modified by Pierre Simon Laplace in 1756. PROTOPLANET HYPOTHESIS. The Solar system formed from a rotating cloud of Gas and Dust (solar nebula). As it rotates conservation of angular momentum caused the cloud to flatten into a disk. 2. Protoplanet hypothesis. Builds on the nebular model but focuses more on the role of planetesimals which then form into full planets. PROCESS: - Small solid particles stick together through collisions. As collisions takes place, it grows into kilometer-sized planetesimals. Gravitational interactions lead to the formation of planets. Lead to formation of steroids belts and varying planet sizes 3. Encounter hypothesis. States that the sun encountered a rogue star. The encounter led to the removal of hot gas from both stars due to their gravitational interaction. The hot gas then accumulated and formed the planets. The materials from the less dense rogue star formed the other planets, while that from the sun formed the inner planets. 4. TIDAL HYPOTHESIS. (also called the Tidal Theory) is an early scientific idea about how the solar system might have formed. Proposed by James Jeans and Harold Jeffreys. A massive star passed very close to the early Sun. The hot gas then accumulated and formed the planets. The materials from the less dense rogue star formed the other planets, while that from the sun formed the inner planets. Streams of hot gas were drawn out from the Sun in elongated shape. These streams eventually condensed and cooled, forming planets, moons, and other bodies in the solar system. 5. Not accepted theory. Later studies showed the streams of hot gas would disperse too quickly into space instead of condensing into planets. The theory also couldn’t explain the specific orbital patterns and compositions we see today. Modern science favors the Nebular Hypothesis, which explains solar system formation through the collapse of a rotating gas cloud. Earth as the only habitable planet 1. Right Distance from the Sun (The Goldilocks Zone). Not too hot, not too cold — just right for liquid water to exist. 2. Atmosphere with Oxygen. Earth has a mix of gases, especially oxygen, which most living things need to survive. 3. Liquid Water. Earth has oceans, rivers, and rain — water is essential for all life. 4. Magnetic Field. Earth’s magnetic field protects us from harmful solar radiation. 5. Stable Climate. The atmosphere and natural cycles keep temperatures and weather mostly stable over time. 6. Rich Resources. Earth has soil for growing food, minerals, and energy sources that support life and technology. Solar explorations 1. AUGUST 6, 2014. First space craft to orbit a comet (ROSETTA PROBE). Captures the comet photograph. -Comets have coma and tail as it approaches to the sun. 2. JULY 14, 2015. NASA’s New Horizons spacecraft made history by becoming the first spacecraft to fly by Pluto, giving us our first close-up look at the dwarf planet. First time visiting Pluto. Before this, Pluto was just a blurry dot in telescope images. Revealed a surprising world New Horizons showed mountains of ice, smooth plains, and a heart-shaped region called Tombaugh Regio. Changed what we knew. Scientists thought Pluto would be dull and frozen — instead, it turned out to be geologically active and incredibly complex. 3. SEPTEMBER 8, 2016. NASA launched OSIRIS-REx, the first U.S. mission to collect a sample from an asteroid and return it to Earth. Changed what we knew. Scientists thought Pluto would be dull and frozen — instead, it turned out to be geologically active and incredibly complex. OSIRIS-REx stands for: Origins, Spectral Interpretation, Resource Identification, Security–Regolith Explorer It was sent to study the asteroid Bennu, a near-Earth asteroid about 500 meters wide. Mission Goals: Collect a sample of surface material from Bennu Study the asteroid’s omposition, structure, and history. Mission Goals: Help scientists understand the origins of the solar system. Learn more about asteroids that could impact Earth. 4. August 12, 2018: Launch of NASA’s Parker Solar Probe, the first spacecraft to "touch" the Sun by flying through its outer atmosphere, called the corona. Mission Goal: To study the Sun up close and help scientists understand: How the solar wind (a stream of charged particles) is formed. Why the Sun’s corona is hotter than its surface. What causes solar storms that can affect Earth’s satellites and power grids. 5. November 26, 2018: NASA’s Insight Lander Touches Down on Mars. Its mission was focused on studying the interior of the Red Planet (crust, mantle, and core of the planet). Why the Sun’s corona is hotter than its surface. What causes solar storms that can affect Earth’s satellites and power grids 6. November 26, 2018: NASA’s Insight Lander Touches Down on Mars. Its mission was focused on studying the interior of the Red Planet (crust, mantle, and core of the planet) 7. JULY 30, 2020 PERSEVERANCE PROBE. Perseverance rover as part of the Mars 2020 mission aboard an Atlas V-541 rocket This marked a major step in Mars exploration. 8. DECEMBER 25, 2021-JAMES WEBB SPACE TELESCOPE. Investigate exoplanets’ atmospheres for signs of habitability. Observe the first galaxies formed after the Big Bang. Study the formation of stars and planetary systems. Look deeper into the infrared universe than ever before. RESULTS OF EXPLORATION • Evidence of Ancient Life-friendly Environment. • Sedimentary rocks formed in water-rich environments. • Signs of clay and carbonate minerals, which can preserve biosignatures (traces of past life). • Evidence of Ancient Life-friendly Environment. • Sedimentary rocks formed in water-rich environments. • Signs of clay and carbonate minerals, which can preserve biosignatures (traces of past life). • Evidence of Ancient Life-friendly Environment. • Sedimentary rocks formed in water-rich environments. • Signs of clay and carbonate minerals, which can preserve biosignatures (traces of past life).

Richard Bland College (RBC), Virginia’s selective, two-year, residential, liberal arts transfer institution, was born through innovation. In 1959, years before the Virginia Community College system was imagined, Frank Ernst – a Gateway region native, entrepreneur, and retired executive of Hopewell’s Allied Chemical Plant – proposed the creation of an institution grounded in the liberal arts tradition with opportunities for specialized training in in-demand fields such as engineering to the State Council of Higher Education. After discussions with Virginia Tech and the University of Virginia, Ernst found a willing partner in the College of William & Mary, the second-oldest university in the United States, who founded Richard Bland College in 1960. RBC has since offered multiple certificates and university-parallel two-year degrees. The College was named for the Virginia statesman and champion of public rights, Richard Bland. Son and grandson of successful planters, Richard Bland was educated at The College of William and Mary. From 1742 until his death in 1776, he represented the area in which the College is now located, first in the House of Burgesses, and later, with the adoption of a state constitution, in the House of Delegates. He also served as a delegate from Virginia in both the First and Second Continental Congresses. It seems fitting, therefore, that an institution of higher learning located in an area served for so many years by this distinguished Virginia patriot and scholar, should derive its name from one whom Jefferson described “as the most learned and logical man of those who took prominent lead in public affairs.” Before the Civil War, the property on which the College is now located was a plantation owned by the Gurley family. It became an important part of the Union-occupied territory during the 1864-1865 Siege of Petersburg. The present campus was the scene of two battles during that campaign. Shortly after the turn of the century, Hatcher Seward established a dairy and cattle farm on the former Gurley property and constructed two farmhouses. Today they serve as the President’s residence and the Hospitality House. In the early 1900s, the still-beautiful grove of pecan trees was planted. The farm was used as a work camp for about twenty conscientious objectors during World War I. The Commonwealth of Virginia authorized Central State Hospital to purchase the land in 1932 for use as the Petersburg Training School and Hospital for African-American Youth. That institution was moved in 1959, and the land, still owned by the Commonwealth, became the location for the establishment of Richard Bland College of The College of William and Mary. Under the guidance of Colonel (Ret.) James M. Carson, the former hospital and training facility was transformed into Richard Bland College, and classes were held beginning in 1961. In the late 1960s, Ernst Hall (named for a local business leader influential in the establishment of the college) was added to the original campus. In addition, a Student Center Library building and a gymnasium also were constructed in the early 1970s. Colonel Carson retired as the founding President of the College in 1973. From 1973 through 1975, Dr. Cornelius Laban, Professor of Biology, Emeritus, served as the Acting President of Richard Bland College. In 1975, Dr. Clarence Maze succeeded Colonel Carson as Richard Bland College’s second President. During his tenure, Richard Bland College expanded its academic programs, added an Asian water garden that was designed by Dr. Maze and expanded international programs and travel. In recognition of his service to the College, the renovated administration building was named Maze Hall upon his retirement in 1996. In 1996, Dr. James B. McNeer succeeded Dr. Clarence Maze as Richard Bland College’s third President. Dr. McNeer introduced a residential life program and oversaw the addition of the Residential Village in 2008. The Residential Village was comprised of two dormitories, Freedom Hall and Patriot Hall, which housed 250 students. A new Science and Technology Building was added in 2010, and in recognition of his service to the College, this building was named James B. McNeer Hall. Dr. McNeer retired in 2012. In 2012, Dr. Debbie L. Sydow succeeded Dr. James McNeer as Richard Bland College’s fourth president. Dr. Sydow expanded the reach, range and diversity of students attending Richard Bland College. She oversaw a physical campus transformation through extensive building renovation and new construction, creation of a Business Innovation Park, and conservation of the iconic pecan grove and water garden. President Sydow reinstituted intercollegiate athletics in 2013 and has since hailed three NJCAA national championship teams. She supported the Foundation’s emergence as a vibrant, entrepreneurial organization led by a Board of Directors composed largely of alumni, and she secured the largest private gift in College history to launch the W&M Promise Scholars program. By effectively leveraging partnerships, President Sydow boosted work-based learning and expanded academic and career pathways for students.

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