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Johann Friedrich Julius Schmidt

Johann Friedrich Julius Schmidt is a astronomy topic covered in the lgStudy science library. This page brings together a partial reference excerpt, illustrations, worked examples, real-world applications and a short study plan, so you can understand Johann Friedrich Julius Schmidt rather than just read about it. In short: Johann Friedrich Julius Schmidt (25 October 1825 in Eutin, Grand Duchy of Oldenburg – 7 February 1884 in Athens, Greece) was a German astronomer and geophysicist. He was the director of the National Observatory of Athens in Greece from 1858 to 1884.

Johann Friedrich Julius Schmidt — main illustration
Johann Friedrich Julius Schmidt — illustration

Key takeaways

  • Johann Friedrich Julius Schmidt belongs to astronomy; place it in that map before memorising details.
  • Learn the definition first, then one example that makes the definition concrete.
  • Connect Johann Friedrich Julius Schmidt to a quantity you can measure, compute or draw — that is where exam questions come from.
  • Reproduce the core statement of Johann Friedrich Julius Schmidt from memory before moving on to harder problems.

Reference excerpt

Johann Friedrich Julius Schmidt (25 October 1825 in Eutin, Grand Duchy of Oldenburg – 7 February 1884 in Athens, Greece) was a German astronomer and geophysicist. He was the director of the National Observatory of Athens in Greece from 1858 to 1884. Julius Schmidt was tireless in his work, it was suggested by William Henry Pickering that he perhaps devoted more of his life than any other man to the study of the Moon. During his lifetime, he made some of the most complete lunar maps of the 19th century. According to his own analysis, he mapped no less than 32,856 craters, with Mädler mapping 7,735 and Lohrmann 7,177. Schmidt also mapped 348 lunar rilles. In six years, he made almost 57,000 micrometer settings to make 3050 height measurements of the terrain.

Biography

Early life Schmidt was born in the town of Eutin to his father Carl Friedrich Schmidt, a glazier and his mother Maria Elisabeth Quirling. He went to school at a gymnasium in Hamburg, where he impressed with his sense of form and drawing abilities and demonstrated a strong interest in science. In the autumn of 1839, during an auction in his hometown, he stumbled upon a copy of Schröter's book, Selenotopographische Fragmente. As Schmidt himself put it, “The sight of numerous illustrations of shadow-casting mountains and craters made such a strong and lasting impression that it determined the main direction of my later life.” Prior to this, 14-year-old Schmidt had been interested in botany and zoology for a while. He could not make the decision to switch careers until he could see for himself what a sight the Moon would grant when viewed through a telescope. That wish was fulfilled when his father made him a "small, very good" telescope which Schmidt used to look at the Moon. Leaning against a lamppost, he recognized the rays of Tycho and immediately made his first attempt at drawing the crater and ray system. This telescope could only magnify 10x, however, the objective was ground according to "Dollond's principle", meaning it was achromatic. Reading Schröter's work and drawing the Moon became his main occupation, and it was not long until Schmidt devised a tripod for the telescope, which could go in both up-down and left-right motions. Although the execution was rough, the wooden mount made it much easier for him to continue lunar observations. Now he started drawing entire phases, not considering the libration but paying attention to the shadows. Thus passed by 1840, with Schmidt's habits making him neglect school. In the spring of 1841, Hellwag, a government councilor who was well experienced in astronomy, noticed his efforts. Hellwag asked Hofrath Voss, the son of the well known Eutin school rector, to entrust Schmidt with a 1200mm focal length Dollond telescope which Schmidt found to be very sharp, approximating the magnification to be 15-20x. He saw the bands of Jupiter, Saturn's rings and a crescent Venus for the first time with it. In July 1841, the Hamburg Gymnasium made a visit to the Altona Observatory, where Schmidt looked through a larger telescope for the first time and became acquainted with the well-known map of the Moon made by Wilhelm Beer and Johann Heinrich Mädler. Dr. Petersen showed him the craters Gassendi and Bullialdus. Rümker taught him the fundamentals of astronomical observation and let him use various telescopes from 1842 to 1845. In 1843, he made his first contribution to Astronomische Nachrichten, about the Sun and variable stars, with many more to follow.

Benzenberg's assistant In 1845, he obtained a position as an assistant at Johann Friedrich Benzenberg's private observatory in Bilk near Düsseldorf, being tasked to with naked eye objects such as meteors, and searching for possible objects closer to the Sun than Mercury. However, the telescope made available to him was practically a low power terrestrial telescope, and the larger instrument was kept under a lock and key, as to prevent 20 year old Schmidt from damaging its "outer looks and splendor". Here, he confined himself to drawing parts of the lunar landscape instead of the entire face, using the method of drawing the same area under different lighting conditions or sun angles, the same one Schröter used. The drawing of entire phases was stopped from this point forward.

Years 1846 – 1858 A year later, after Benzenberg died, he joined the Bonn Observatory under Friedrich Wilhelm Argelander. Here, Schmidt measured the visual magnitudes and positions for Hora V of the Berlin Academy of Sciences star chart and catalogue project. He was not able to continue observing the Moon due to his job, but he still obtained numerous valuable drawings, and when he did not, what was seen was preserved in writing. He left Bonn in May of 1853 due to ill health. He received an honorary doctorate from Bonn in 1868. From 1853 to 1858 he was director of Baron von Unkrechtsberg's private observatory at Olmütz (today Olomouc, Czech Republic), where he made only a few drawings, but undertook micrometric measurements of its mountains to further increase the knowledge of the Moon.

Work at Athens Observatory In 1858, Simon Sinas made a proposal for Schmidt to come to Athens and become the director of the Athens Observatory (now known as National Observatory of Athens). Accepting the offer would bring him a good salary, freedom to do the research he wants to do and a site with a large amount of clear nights per year. The decision was his, as Schmidt never married, so on December 2, he chose to accept the offer. The degraded state of the observatory forbid observation. It was not until November 1859 that it was in a usable state, after a year of repairs requested by Schmidt, though the restoration was entirely completed in 1861. The observatory's instruments at the time included:

… excerpt ends here. Continue reading the full article.

Illustrations

Johann Friedrich Julius Schmidt illustration
Johann Friedrich Julius Schmidt: A photo of Julius Schmidt
A photo of Julius Schmidt
Johann Friedrich Julius Schmidt: Field Columbian Museum Moon Model, made by Julius Schmidt and Thomas Dickert in 1854
Field Columbian Museum Moon Model, made by Julius Schmidt and Thomas Dickert in 1854
Johann Friedrich Julius Schmidt: Title page of the chart
Title page of the chart
Johann Friedrich Julius Schmidt illustration

Worked examples

Example 1 — a first encounter with Johann Friedrich Julius Schmidt

Start with the simplest possible case. Write down what Johann Friedrich Julius Schmidt claims or describes in one sentence, then invent the smallest concrete situation in which that sentence is true. In astronomy, the smallest case is usually a single object, a single equation or a single measurement. Check that every symbol or term in your sentence has a meaning in that case.

Example 2 — changing one variable

Take the situation from Example 1 and change exactly one quantity: double it, halve it, or set it to zero. Predict what should happen to Johann Friedrich Julius Schmidt before you calculate. Comparing your prediction with the result is the fastest way to find out whether you understand the idea or only the words.

Example 3 — an exam-style question

Typical questions about Johann Friedrich Julius Schmidt ask you to (a) state it precisely, (b) apply it to given data, and (c) explain a limitation. Practise writing all three answers in under five minutes; the third part is what separates a full-mark answer from an average one.

Applications of Johann Friedrich Julius Schmidt

In research
Johann Friedrich Julius Schmidt appears in astronomy research whenever the underlying quantities have to be modelled precisely. Papers usually cite it as a starting assumption and then explore where it breaks down.
In technology and industry
Engineering practice reuses Johann Friedrich Julius Schmidt in design rules, simulations and safety margins. Knowing the idea lets you read a specification sheet and understand why the numbers look the way they do.
In the classroom
Johann Friedrich Julius Schmidt is common in secondary-school and first-year university syllabi. It links to neighbouring topics 1825 births, 1884 deaths, 19th-century German astronomers, so understanding it makes those chapters shorter.
In everyday life
Look for Johann Friedrich Julius Schmidt outside the textbook — in sport, cooking, traffic, electronics or the sky above you. An example you found yourself is remembered far longer than one you were given.
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How to study Johann Friedrich Julius Schmidt in 20 minutes

  1. Read the reference excerpt below once, without taking notes.
  2. Close the page and write down what Johann Friedrich Julius Schmidt means in your own words.
  3. Compare your version with the excerpt and mark what you missed.
  4. Work through the three examples above with pen and paper.
  5. Explain Johann Friedrich Julius Schmidt out loud to somebody else — or to Teacher Smith in the lgStudy chat.

Frequently asked questions

What is Johann Friedrich Julius Schmidt in simple terms?

Johann Friedrich Julius Schmidt (25 October 1825 in Eutin, Grand Duchy of Oldenburg – 7 February 1884 in Athens, Greece) was a German astronomer and geophysicist. He was the director of the National Observatory of Athens in Greece from 1858 to 1884.

Why does Johann Friedrich Julius Schmidt matter?

Because it connects several astronomy ideas at once: it gives you a definition you can apply, a quantity you can calculate, and a way to check whether a result is plausible.

How should I study Johann Friedrich Julius Schmidt?

Read the excerpt, restate it from memory, then work through the examples and applications listed on this page. The five-step study plan above takes about twenty minutes.

What does this page cover?

It gives you a compact reference excerpt plus original lgStudy explanations, examples, applications and study material on Johann Friedrich Julius Schmidt.

Tags

  • 1825 births
  • 1884 deaths
  • 19th-century German astronomers
  • 19th-century Greek astronomers
  • Academic staff of the University of Bonn
  • Discoverers of comets
  • People from Eutin
  • People from the Grand Duchy of Oldenburg
  • Selenographers

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