Sun-Earth Day

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Sun-Earth Day is a joint educational program established in 2000 by NASA and ESA. The goal of the program is to popularize the knowledge about the Sun, and the way it influences life on Earth, among students and the public. [1] The day itself is mainly celebrated in the United States near the time of the spring equinox. However, the Sun-Earth Day event actually runs throughout the year, with a different theme being chosen each year. [2]

Contents

Themes

The selection of each year's theme often corresponds to events for that year. [3] Every theme is supported by free educational plans for both informal and formal educators. [2] Here is a list of themes by year:

Sun-Earth Day (Themes)
YearDateTheme
2001 Having a Solar Blast
2002 Celebrate the Equinox
2003 Live from the Aurora
2004 Venus Transit
2005 Ancient Observatories Timeless Knowledge
2006 Eclipse: In a Different Light
2007 Living in the Atmosphere of the Sun
2008 Space Weather Around the World
2009 Our Sun, Yours to Discover
2010 Magnetic Storms
2011 March 19, 2011 Ancient Mysteries; Future Discoveries. [4]
2012 June 5, 2012 Transit of Venus [5]
2013 Solar Max – Storm Warning! [6]
2014 [ data unknown/missing ]
2015 [ data unknown/missing ]
2016 [ data unknown/missing ]
2017 [ data unknown/missing ]

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<span class="mw-page-title-main">Mercury (planet)</span> First planet of the Solar System

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Pioneer program Series of United States uncrewed lunar and planetary space probes (1958-60; 1965-92)

The Pioneer programs were two series of United States lunar and planetary space probes exploration. The first program, which ran from 1958 to 1960, unsuccessfully attempted to send spacecraft to orbit the Moon, successfully sent one spacecraft to fly by the Moon, and successfully sent one spacecraft to investigate interplanetary space between the orbits of Earth and Venus. The second program, which ran from 1965 to 1992, sent four spacecraft to measure interplanetary space weather, two to explore Jupiter and Saturn, and two to explore Venus. The two outer planet probes, Pioneer 10 and Pioneer 11, became the first of five artificial objects to achieve the escape velocity that will allow them to leave the Solar System, and carried a golden plaque each depicting a man and a woman and information about the origin and the creators of the probes, in case any extraterrestrials find them someday.

<span class="mw-page-title-main">Venus</span> Planet

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Conjunction (astronomy) When two astronomical objects have the same right ascension or the same ecliptic longitude

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<span class="mw-page-title-main">Solar and Heliospheric Observatory</span> European space observatory

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<i>MESSENGER</i> Seventh mission of the Discovery program; orbital reconnaissance of the planet Mercury (2004–2015)

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Transit of Venus Astronomical transit of Venus across the Sun

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Transit of Mercury Movement of Mercury across the Sun from an astronomers perspective

A transit of Mercury across the Sun takes place when the planet Mercury passes directly between the Sun and a superior planet. During a transit, Mercury appears as a tiny black dot moving across the Sun as the planet obscures a small portion of the solar disk. Because of orbital alignments, transits viewed from Earth occur in May or November. The last four such transits occurred on May 7, 2003; November 8, 2006; May 9, 2016; and November 11, 2019. The next will occur on November 13, 2032. A typical transit lasts several hours. Mercury transits are much more frequent than transits of Venus, with about 13 or 14 per century, primarily because Mercury is closer to the Sun and orbits it more rapidly.

2012 transit of Venus Transit of Venus across the Sun visible from Earth on 5–6 June 2012

The 2012 transit of Venus, when the planet Venus appeared as a small, dark spot passing across the face of the Sun, began at 22:09 UTC on 5 June 2012, and finished at 04:49 UTC on 6 June. Depending on the position of the observer, the exact times varied by up to ±7 minutes. Transits of Venus are among the rarest of predictable celestial phenomena and occur in pairs. Consecutive transits per pair are spaced 8 years apart, and consecutive pairs occur more than a century apart: The previous transit of Venus took place on 8 June 2004 ; the next pair of transits will occur on 10–11 December 2117 and December 2125 within the 22nd century.

Transit of Phobos from Mars Transit of a Moon from Mars

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<span class="mw-page-title-main">Observations and explorations of Venus</span>

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<span class="mw-page-title-main">Solar eclipse</span> Natural phenomenon wherein the Sun is obscured by the Moon

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Atmosphere of Venus Gas layer surrounding Venus

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Syzygy (astronomy) Configuration of celestial bodies

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Kepler-62d is the third innermost and the largest exoplanet discovered orbiting the star Kepler-62, with a size roughly twice the diameter of Earth. It was found using the transit method, in which the dimming that a planet causes as it crosses in front of its star is measured. Its stellar flux is 15 ± 2 times Earth's. Due to its closer orbit to its star, it is a super-Venus or, if it has a volatile composition, a hot Neptune, with an estimated equilibrium temperature of 510 K, too hot to sustain life on its surface.

References

  1. "Sun-Earth Day 2004: Transit of Venus". Science Scope. National Science Teachers Association. 27 (5): 34–41. Feb 2004. ProQuest   226011597.
  2. 1 2 "Sun Earth Day web page".
  3. "Past Sun-Earth Days 2012" . Retrieved 2012-04-19.
  4. "Goddard Annual Sun-Earth Day Has a Tweeting Twist". NASA. 6 June 2013.
  5. Thieman, James. "Venus Transit: About Sun-Earth Day 2012" . Retrieved 2012-04-19.
  6. "Solar Maximum 2013". NASA. Retrieved 2013-01-11.