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[Jerica Shilt]

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You may qualify for one of these programs based on your income. Talk with your medical provider about the best birth control option for you. Find out if you qualify for free birth control by registering as a patient at Daily Planet Health Services. You may register by phone by calling (804) 783-2505. Click here for more information on this process.

Descubra si califica para anticonceptivos gratis al registrarse como paciente de Daily Planet Health Services. Puedes regstrese por telfono llamando al (804) 783-2505. Visite a dailyplanetva.org/patientregistration para ms informacin.

A guiding principle of Daily Planet Health Services is our belief that ALL should have access to quality health services regardless of their financial, housing, citizenship, or insurance status. Our philosophy is that healthcare is a right for all and not a privilege for the few.

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Planet Explorer is an online tool used to search and analyze geospatial imagery, allowing you to see change across the planet over time. You can use Planet Explorer to search through an imagery catalog and either download full-resolution data or analyze hosted data in the browser.

Download Daily Scenes: You can download daily scenes by ordering directly from the app or by sourcing cURL requests for specific scene IDs if you prefer the API. You must purchase a plan to do so.

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Our Plant-Based Coconut-Based Shredded Cheddar and Mozzarella, and Plant-Based Sliced American, Pepper Jack, Cheddar, and Smoked Provolone are all certified Keto. Our Snackable Wedges and Real Smoked Wheels are also all certified Keto.

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SpaceEngine is a realistic virtual Universe you can explore on your computer. You can travel from star to star, from galaxy to galaxy, landing on any planet, moon, or asteroid with the ability to explore its alien landscape. You can alter the speed of time and observe any celestial phenomena you please. All transitions are completely seamless, and this virtual universe has a size of billions of light-years across and contains trillions upon trillions of planetary systems. The procedural generation is based on real scientific knowledge, so SpaceEngine depicts the universe the way it is thought to be by modern science. Real celestial objects are also present if you want to visit them, including the planets and moons of our Solar system, thousands of nearby stars with newly discovered exoplanets, and thousands of galaxies that are currently known.

Click on any visible object with the mouse and hit the 'G' key to fly directly to it. Search for objects by name, search by parameters within a certain radius, browse an interactive map of the surrounding space and view a map of the current planetary system

At the moment, we are no longer accepting donations via PayPal. If you want to support SpaceEngine beyond purchasing it for yourself, consider buying a copy for a friend or simply tell your friends and family about SpaceEngine and why you love it. No matter what you do, we deeply appreciate your support!

A rogue planet, also termed a free-floating planet (FFP) or an isolated planetary-mass object (iPMO), is an interstellar object of planetary mass which is not gravitationally bound to any star or brown dwarf.[1][2][3][4]

Rogue planets may originate from planetary systems in which they are formed and later ejected, or they can also form on their own, outside a planetary system. The Milky Way alone may have billions to trillions of rogue planets, a range the upcoming Nancy Grace Roman Space Telescope will likely be able to narrow.[5][6]

The two first discovery papers use the names isolated planetary-mass objects (iPMO)[9] and free-floating planets (FFP).[10] Most astronomical papers use one of these terms.[11][12][13] The term rogue planet is more often used for microlensing studies, which also often uses the term FFP.[14][15] A press release intended for the public might use an alternative name. The discovery of at least 70 FFPs in 2021, for example, used the terms rogue planet,[16] starless planet,[17] wandering planet[18] and free-floating planet[19] in different press releases.

Isolated planetary-mass objects (iPMO) were first discovered in 2000 by the UK team Lucas & Roche with UKIRT in the Orion Nebula.[10] In the same year the Spanish team Zapatero Osorio et al. discovered iPMOs with Keck spectroscopy in the σ Orionis cluster.[9] The spectroscopy of the objects in the Orion Nebula was published in 2001.[20] Both European teams are now recognized for their quasi-simultaneous discoveries.[21] In the year 1999 the Japanese team Oasa et al. discovered objects in Chamaeleon I[22] that were spectroscopically confirmed years later in 2004 by the US team Luhman et al.[23]

In October 2023, based on observations of the Orion Nebula with the James Webb Space Telescope, astronomers reported the discovery of pairs of rogue planets, similar in mass to the planet Jupiter, called Jupiter Mass Binary Objects (JuMBOs).[24][25]

Astrophysicist Takahiro Sumi of Osaka University in Japan and colleagues, who form the Microlensing Observations in Astrophysics and the Optical Gravitational Lensing Experiment collaborations, published their study of microlensing in 2011. They observed 50 million stars in the Milky Way by using the 1.8-metre (5 ft 11 in) MOA-II telescope at New Zealand's Mount John Observatory and the 1.3-metre (4 ft 3 in) University of Warsaw telescope at Chile's Las Campanas Observatory. They found 474 incidents of microlensing, ten of which were brief enough to be planets of around Jupiter's size with no associated star in the immediate vicinity. The researchers estimated from their observations that there are nearly two Jupiter-mass rogue planets for every star in the Milky Way.[26][27][28] One study suggested a much larger number, up to 100,000 times more rogue planets than stars in the Milky Way, though this study encompassed hypothetical objects much smaller than Jupiter.[29] A 2017 study by Przemek Mrz of Warsaw University Observatory and colleagues, with six times larger statistics than the 2011 study, indicates an upper limit on Jupiter-mass free-floating or wide-orbit planets of 0.25 planets per main-sequence star in the Milky Way.[30]

In September 2020, astronomers using microlensing techniques reported the detection, for the first time, of an Earth-mass rogue planet (named OGLE-2016-BLG-1928) unbound to any star and free floating in the Milky Way galaxy.[15][31][32]

Astronomers have used the Herschel Space Observatory and the Very Large Telescope to observe a very young free-floating planetary-mass object, OTS 44, and demonstrate that the processes characterizing the canonical star-like mode of formation apply to isolated objects down to a few Jupiter masses. Herschel far-infrared observations have shown that OTS 44 is surrounded by a disk of at least 10 Earth masses and thus could eventually form a mini planetary system.[41] Spectroscopic observations of OTS 44 with the SINFONI spectrograph at the Very Large Telescope have revealed that the disk is actively accreting matter, similar to the disks of young stars.[41]

In the Orion Nebula a population of 40 wide binaries and 2 triple systems were discovered. This was surprising for two reasons: The trend of binaries of brown dwarfs predicted a decrease of distance between low mass objects with decreasing mass. It was also predicted that the binary fraction decreases with mass. These binaries were named Jupiter-mass binary objects (JuMBOs). They make up at least 9% of the iPMOs and have a separation smaller than 340 AU. It is unclear how these JuMBOs formed, but an extensive study argued that they formed in situ, like stars.[42] If they formed like stars, then there must be an unknown "extra ingredient" to allow them to form. If they formed like planets and were later ejected, then it has to be explained why these binaries did not break apart during the ejection process.[25] Future proper motion measurements with JWST might resolve if these objects formed as ejected planets or as stars. Ejected planets should show a high proper motion, while a formation like stars should show proper motions similar to the Trapezium Cluster stars.

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