10 March 1977

Astronomers discover the rings of Uranus.

The rings of Uranus are a system of narrow, dark rings encircling the planet Uranus. They were first discovered in 1977 by astronomers James L. Elliot, Edward W. Dunham, and Douglas J. Mink using the Kuiper Airborne Observatory. At that time, the rings were observed as faint lines passing in front of a star as Uranus occulted it.

Astronomers have identified 13 distinct rings around Uranus, which are named in order of their discovery. The rings are primarily composed of dark particles, likely made up of water ice, dust, and rocky debris. These particles range in size from micrometers to a few meters across.

The rings of Uranus are much darker than those of Saturn, for example, which are predominantly made up of bright ice particles. This darkness is believed to be due to the presence of organic compounds, possibly formed from the bombardment of the rings by charged particles from the Sun and Uranus’s magnetosphere.

The rings of Uranus are thought to be relatively young compared to those of other gas giants like Saturn. They may have formed from the breakup of one or more small moons or from the collision of larger bodies in Uranus’s system. The exact mechanisms of their formation and evolution are still topics of ongoing research.

Observations from space probes like Voyager 2, which flew by Uranus in 1986, have provided valuable insights into the rings’ characteristics and structure. Future missions to Uranus, such as the proposed Uranus Orbiter and Probe mission, could further enhance our understanding of these enigmatic rings.

10 March 2000

The Dot-com bubble peaks with the NASDAQ Composite stock market index reaching 5,048.62.

The Dot-com bubble was a period of excessive speculation in Internet-related companies and their stocks in the late 1990s and early 2000s. During this time, many investors were pouring large amounts of money into companies that had little or no earnings, but were expected to become profitable in the future. The rapid growth of the Internet, combined with the excitement and hype surrounding new technologies, fueled this speculative fervor.

As more and more investors piled into these companies, their stock prices soared to unprecedented levels, often far beyond their intrinsic value. However, the bubble eventually burst in the early 2000s, as many of these companies failed to meet expectations and the market corrected itself. This led to a widespread market downturn and many of the companies that were previously highly valued lost much of their worth, resulting in large losses for investors.

The Dot-com bubble was a significant event in the history of the stock market and serves as a reminder of the potential dangers of excessive speculation and hype.

10 March 1848

The Treaty of Guadalupe Hidalgo is ratified by the United States Senate which ends the Mexican–American War.

California and New Mexico were quickly occupied by American forces in the summer of 1846, and fighting there ended on 13 January 1847 with the signing of the “Capitulation Agreement” at “Campo de Cahuenga” and end of the Taos Revolt. By the middle of September 1847, U.S. forces had successfully invaded central Mexico and occupied Mexico City.

Peace negotiations
Some Eastern Democrats called for complete annexation of Mexico and claimed that some Mexican liberals would welcome this, but President Polk’s State of the Union address in December 1847 upheld Mexican independence and argued at length that occupation and any further military operations in Mexico were aimed at securing a treaty ceding California and New Mexico up to approximately the 32nd parallel north and possibly Baja California and transit rights across the Isthmus of Tehuantepec.

Despite its lengthy string of military defeats, the Mexican government was reluctant to agree to the loss of California and New Mexico. Even with its capital under enemy occupation, the Mexican government was inclined to consider factors such as the unwillingness of the U.S. administration to annex Mexico outright and what appeared to be deep divisions in domestic U.S. opinion regarding the war and its aims, which gave it reason to conclude that it was actually in a far better negotiating position than the military situation might have suggested. A further consideration was the Mexican government’s opposition to slavery and its awareness of the well-known and growing sectional divide in the U.S. over the issue of slavery. It therefore made sense for Mexico to negotiate with a goal of pandering to Northern U.S. interests at the expense of Southern U.S. interests.

The Mexicans proposed peace terms that offered only sale of Alta California north of the 37th parallel north — north of Santa Cruz, California and Madera, California and the southern boundaries of today’s Utah and Colorado. This territory was already dominated by Anglo-American settlers, but perhaps more importantly from the Mexican point of view, it represented the bulk of pre-war Mexican territory north of the Missouri Compromise line of parallel 36°30? north — lands that, if annexed by the U.S., would have been presumed by Northerners to be forever free of slavery. The Mexicans also offered to recognize the U.S. annexation of Texas, but held to its demand of the Nueces River as a boundary.

While the Mexican government could not reasonably have expected the Polk Administration to accept such terms, it would have had reason to hope that a rejection of peace terms so favorable to Northern interests might have the potential to provoke sectional conflict in the United States, or perhaps even a civil war that would fatally undermine the U.S. military position in Mexico. Instead, these terms combined with other Mexican demands only provoked widespread indignation throughout the U.S. without causing the sectional conflict the Mexicans were hoping for.

Jefferson Davis advised Polk that if Mexico appointed commissioners to come to the U.S., the government that appointed them would probably be overthrown before they completed their mission, and they would likely be shot as traitors on their return; so that the only hope of peace was to have a U.S. representative in Mexico. Nicholas Trist, chief clerk of the State Department under President Polk, finally negotiated a treaty with the Mexican delegation after ignoring his recall by President Polk in frustration with failure to secure a treaty. Notwithstanding that the treaty had been negotiated against his instructions, given its achievement of the major American aim, President Polk passed it on to the Senate.

A section of the original treaty
The Treaty of Guadalupe Hidalgo was signed by Nicholas Trist and Luis G. Cuevas, Bernardo Couto and Miguel Atristain as plenipotentiary representatives of Mexico on 2 February 1848, at the main altar of the old Basilica of Guadalupe at Villa Hidalgo as U.S. troops under the command of Gen. Winfield Scott were occupying Mexico City.

Changes to the treaty and ratification
The version of the treaty ratified by the United States Senate eliminated Article X, which stated that the U.S. government would honor and guarantee all land grants awarded in lands ceded to the U.S. to citizens of Spain and Mexico by those respective governments. Article VIII guaranteed that Mexicans who remained more than one year in the ceded lands would automatically become full-fledged United States citizens; however, the Senate modified Article IX, changing the first paragraph and excluding the last two. Among the changes was that Mexican citizens would “be admitted at the proper time” instead of “admitted as soon as possible”, as negotiated between Trist and the Mexican delegation.

An amendment by Jefferson Davis giving the U.S. most of Tamaulipas and Nuevo León, all of Coahuila and a large part of Chihuahua was supported by both senators from Texas, Daniel S. Dickinson of New York, Stephen A. Douglas of Illinois, Edward A. Hannegan of Indiana, and one each from Alabama, Florida, Mississippi, Ohio, Missouri and Tennessee. Most of the leaders of the Democratic party, Thomas Hart Benton, John C. Calhoun, Herschel V. Johnson, Lewis Cass, James Murray Mason of Virginia and Ambrose Hundley Sevier were opposed and the amendment was defeated 44–11.

An amendment by Whig Sen. George Edmund Badger of North Carolina to exclude New Mexico and California lost 35–15, with three Southern Whigs voting with the Democrats. Daniel Webster was bitter that four New England senators made deciding votes for acquiring the new territories.

A motion to insert into the treaty the Wilmot Proviso failed 15–38 on sectional lines.

The treaty was subsequently ratified by the U.S. Senate by a vote of 38 to 14 on 10 March 1848 and by Mexico through a legislative vote of 51 to 34 and a Senate vote of 33 to 4, on 19 May 1848. News that New Mexico’s legislative assembly had just passed an act for organization of a U.S. territorial government helped ease Mexican concern about abandoning the people of New Mexico. The treaty was formally proclaimed on 4 July 1848.

10 March 1977

Astronomers discover the rings of the planet Uranus.

For being the third largest body in our solar system not including the Sun, there really wasn’t much info about Uranus until the invention of powerful modern telescopes. While astronomers have known of it’s existence since the 16th century, it wasn’t until 1781 that Englishman William Hershel confirmed it as the seventh planet from the sun.

Named after Zeus’s grandfather Uranus, best remembered for being castrated by his son Saturn, the hilariously named planet was only a blue blip until 1977. Astronomers using the Kuiper Airborne Observatory discovered a series of rings the circled Uranus around it’s uniquely tilted axis. This marked the second such celestial feature alongside fellow gas giant Saturn.

Years later the solar system observer Voyager arrived near Uranus and confirmed that Uranus not only had a complicated system of rings, but also 27 moons of various sizes. With a new discovery at every turn the question remains, what new wonders does Uranus have in store for us next?

10 March 1977

Astronomers discover the rings of Uranus.

The rings of Uranus were first discovered in 1977 by the astronomical team of James L. Elliot, Edward W. Dunham, and Douglas J. Mink. When he first discovered Uranus more than 200 years ago, William Herschel also reported seeing rings, but that’s probably impossible, because the rings of Uranus are very dark and thin.

Astronomers now know that Uranus has 13 distinct rings. They start at about a distance of 38,000 km from the center of Uranus, and then extend out to about 98,000 km.Unlike the rings of Saturn, which are very bright and composed of water ice, the rings of Uranus are relatively dark. Instead of containing dust, the rings seem to be made up of larger chunks, measuring 0.2 to 20 m across. These would really qualify as boulders, not dust. They’re also very thin. Each ring is only a few km thick.

Uranus now has a total of 10 known rings.The rings of Uranus are thought to be very young, not more than 600 million years old. They probably came from a few shepherd moons that were shattered by Uranus’ gravity and turned into rings around the planet. The chunks collided with each other and turned into smaller and smaller particles.